NIST 5 miner
Publish: 2021-04-25 18:39:27
1. Unknown_Error
2.
mining proficiency of world of Warcraft:
1. First, learn mining skills and acquire the skill of "looking for minerals". Nearby minerals will be displayed on the small map
3.
There are five meanings
1, the brand Neo of Adidas
Adidas Neo belongs to Adidas sports and leisure series, which is the freshest sports and leisure brand integrated into your daily life. Adidas Neo means fresh and energetic, full of optimism, full of movement, personal affinity, fresh and advancing with the times
2, Neo (Polish eSports)
Polish eSports. In 2012, Neo played an outstanding role in the super death group, and fought with the Ukrainian emperor Na ` VI to win the IEM world finals. In September of the same year, it announced the formal transformation of CS: go. After hard training, ESC team finally won the first championship after the transformation of CS: go at the end of 2012
The most frightening thing about Neo is that it will eat all the creatures in front of it. Neo's belly is completely another world, and being swallowed by it is equivalent to permanent disappearance. Although Neo has also died, it will always come back to life. No matter how powerful the opponent is, it will be doomed. Neo is a nightmare forever. In short, the most terrible thing about Neo is not strength, but endless appetite Neo, also known as pirate boss, is 1000 years old and 2 meters tall. He is the boss of the space pirate Obi organization and the captain of the ghost. He first appeared in the mission "decisive battle with the ghost", and is one of the biggest enemies of the sail. He has four capable generals: bit, Zog, Alison and Dean (later betrayed)5, Neo (contact lens brand)
Neo, Chinese name "anthracene Yiao". It is affiliated to Neo vision company of South Korea. Neo vision is one of the largest stealth companies in South Korea. It has repeatedly won the championship in terms of stealth sales in Japan and South Korea. Neo vision's contact lenses occupy 80% of South Korea's lens market
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extended materials:
on November 27, 2017, Adidas Neo officially announced that the new generation of youth idol, e-close Qianxi, has become Adidas Neo's new brand spokesman and the first global youth creative officer
As a global youth representative, Yixiang Qianxi will give full play to its creative inspiration and bring more unexpected surprises to the global youth group together with Adidas Neo. In the future, Adidas Neo will join hands with Yiguan Qianxi to create more exciting "born active" brand activities, and share more active vitality and new experience with young groups4. Rox and Vega squadron have been warned] vaevictis eSports have launched an all women's team in the LCL League. However, the women's team's performance is not ideal, and other teams in various forms of fancy sling. For example, when the Rox team was at BP, ban provided five AIDS, while Vega squadron deliberately prolonged the game and did not take the initiative to end the game. Not long ago, however, both teams were warned by fists for disrespect for sportsmanship and discrimination against women< Riot said that gender discrimination and any other type of discrimination should not exist and should not be accepted at all. He hoped that all teams would show sincerity and respect for their opponents in the competition. Therefore, Rox and Vega squadron were warned, which means that if such violations happen again, they will be punished more seriously.
5. Asteroids are members of the solar system family. Their "size" is much smaller than the satellites of major planets. They are generally distributed in the asteroid belt, which is between the orbits of Mars and Jupiter. They are characterized by small size and small mass. The largest asteroid is less than 800 kilometers in diameter. Like the big planets, they orbit the sun in an elliptical orbit. Since Italian astronomer Piazzi accidentally discovered the first asteroid Ceres in 1801, tens of thousands of asteroids have been discovered. By the end of 1994, more than 5300 asteroids had been officially registered and obtained the "citizenship" of the solar family
although asteroids are very small, they have played an important role in previous astronomical studies. For example, in 1873, the German astronomer gale used the No. 8 Venus to rush to the sun, and in 1877, the British astronomer Jill used the No. 4 Vesta to rush to the sun to determine the distance between the sun and the earth, both of which obtained accurate results. From 1930 to 1931, ring the great rush of Eros 433, the International Astronomical Union organized an international joint survey on an unprecedented scale, and obtained the most accurate value of sun earth distance that can be achieved by triangulation, which is 149.58 million km< In addition, asteroids can be used to determine the mass of planets. When an asteroid approaches a major planet, the perturbation of the major planet will inevitably affect its orbit, and the actual mass of the planet can be calculated from the tiny change of its orbit. In 1870, the mass of Jupiter was 1 / 1047 of the mass of the sun, which was measured by astronomers when emfitletta approached Jupiter on the 29th. Today, astronomers still use this number. The mass of mercury, Venus, Saturn, Mars and other planets are measured by asteroids, and the measured values have a high accuracy
in order to improve and improve the accuracy of the catalogue, the International Astronomical Union (IAU) has organized more than ten observatories to conct long-term monitoring and rection of Ceres and other 10 asteroids, and obtain the accurate positions of the ecliptic and celestial equator from the actual data and known orbital elements
asteroids also provide important clues for the study of the origin and evolution of the solar system. According to the modern theory of the formation of the solar system, the solar system was formed by a cluster of chaotic nebulae 4.6 billion years ago. However, the specific process of the formation of the solar system by nebulae can no longer be traced from the earth or other planets. Only asteroids and comets still retain many of the early states of the solar system, so they are called "living fossils" of the early solar system by astronomers
in addition, asteroid research is of great significance for the development of human space instry, the protection of the earth's environment and the development of the universe. In particular, near Earth Asteroids, which are not only potential mineral resources, but also the most easily realized target of space exploration among asteroids
the diameter of asteroids is very small. In the radius values of hundreds of asteroids obtained by astronomers, only a few larger and closer asteroids are measured directly, and the others are measured by infrared wave and polarization method. Measurements show that there are about 110 asteroids with a diameter of more than 100 km, and about 560 asteroids with a diameter of more than 50 km. Most of the asteroids have a diameter of 1-2 km, which is not as big as a mountain on earth
as for the mass of asteroids, except Ceres No.1, Ares No.2 and Vesta No.4, the mass of all asteroids is calculated by their diameter and assumed density, and only the concept of order of magnitude. It is generally believed that the total mass of asteroids is 100 billion tons, of which Ceres accounts for about half of the total mass
the albedo of asteroids depends on their chemical composition and surface conditions. Because of the different albedo of each part of the asteroid surface and its rotation, the brightness of the asteroid changes periodically. According to the brightness curve, the rotation period and the orientation of the rotation axis of asteroids can be measured, and their shapes can be inferred. Judging from more than 200 known asteroids, most of them have rotation periods of 4-16 hours, with an average of 11.47 hours. The orientation of the rotation axis is randomly distributed. Asteroids larger than 100 km in diameter are generally regular in shape, close to spherical, while asteroids smaller than 100 km in diameter are various in shape, some are long cylindrical, some are like mbbells, and some are even like two stones stuck together
since the end of 1950s, the Zijinshan Observatory in China has published dozens of asteroid luminosity curves, some of which were first published in the world. Due to the high observation quality, they have been widely used by foreign observers< On October 29, 1991, the Galileo spacecraft passed the 951 asteroid gaspa and approached the asteroid at a distance of 1600 km. The detailed features of the asteroid's surface of 50 meters can be clearly seen. Preliminary measurements by the near-infrared mapping spectrometer on board the spacecraft show that Gaspar's shape is very irregular and may have been split from a large matrix. This is the first asteroid detected by the spacecraft< In August 1993, Galileo flew by 243 IDA, making it the second asteroid visited by a spacecraft. Gaspra and Ida are both metal rich and belong to S-type asteroids< On June 27, 1997, near and 253 Mathilde passed by. This is the first time that scientists have been able to observe the carbon rich C-type asteroid at close range. This visit is the only one because near detector is not specially used to investigate it. Near was used to investigate Eros asteroid in January 1999
many asteroids have been observed on the ground by astronomers. Some famous asteroids include toutais, Castalia, Vesta and geographes. For the asteroids touratis, Castalia and geographes, astronomers study them on the ground through radio observations when they approach the sun. Vesta was discovered by the Hubble Space Telescope. At present, Italy has developed a space exploration program for near Earth Asteroids named Piazzi, preparing to explore Eros near earth< On June 7, 1978, American astronomer McMahon discovered a satellite named 1978 (532) I when he observed 532 Hercules to cover its star. This is the first time that astronomers have discovered an asteroid with a satellite. Asteroid 532 and its satellite are 243 km and 45.6 km in diameter, 977 km apart from each other. Half a year later, astronomers discovered that there are satellites in Yushen star 18 from the data of its star covering. The center distance of the two small objects is 460 km, and the diameter is 135 km and 37 km respectively. If this is a synchronous satellite, the angular diameter of the "Moon" on Yushen star can reach 5 ° Its apparent area is almost 120 times that of our moon. Later, when reprocessing the occultation data of some asteroids in the past, it was found that a number of asteroids also had satellites, including Zhishen No. 2, Chunshen No. 6, Haishen No. 9 and kaishen No. 12, with about 30 to 40 satellites< In 1980, U.S. astronomers used the new technology of spot interferometry to prove that there was indeed a satellite in Zhishen 2. However, the issue of whether there was a satellite in asteroid remains unresolved. Some astronomers who hold opposing opinions believe that human beings have launched so many space probes, but so far no asteroid satellite has been found, So the conclusion that asteroids have satellites lacks observational evidence. In addition, there is no final conclusion about the level of asteroid satellites in the celestial system and whether they can be compared with the moon or Ganymede< In October 1991, Galileo, the Jupiter probe launched in 1989, flew past Gaspar, the 951 asteroid, fulfilling Astronomers' dream of exploring asteroids. In August 1993, "Galileo" swept over IDA, the No. 243 asteroid, and made a number of observations. In February 1994, astronomers analyzed the data sent back by Galileo and found that there was a much smaller satellite near IDA. They published a group photo of IDA and the satellite and a magnified image of the satellite in the British academic weekly nature. Since then, Galileo has sent back updated imaging and spectral data. According to this, astronomers estimated that the diameter of IDA satellite was 1.5 km, and the discovery time was only 100 km away from the asteroid. Astronomers believe that this is the first case of the discovery of an asteroid with a satellite<
the orbital distribution of asteroids
the orbits of asteroids are oval, about 95% of the asteroids' orbits are between 2.17 and 3.64 astronomical units. This space area is called the main belt of asteroids, and the asteroids in the main belt are called "main belt asteroids"
a small number of asteroids are isolated and form several special groups. Distant asteroids with orbital radii greater than 3.3 astronomical units are called distant asteroids. Among them, the most famous is the Toro central group, whose orbital radii are as large as those of Jupiter. From the sun, there are some 60 years ahead of Jupiter °， Some are 60 years behind Jupiter °， The former is called "Greek group", and the latter is called "pure Toro central group"
another special group is near Earth Asteroids, whose orbit perihelions go deep into the inner solar system, and some even run into the earth's orbit, which is called near Earth Asteroids. According to the numerical characteristics of the distance and half major diameter of the orbit perihelion, the near earth asteroids are divided into amore type, Apollo type and Arden type
the orbital characteristics of amore asteroids are that the perihelion is within the orbit of Mars - 1.02-1.3 astronomical units, the half major diameter is 1.39-4.23 astronomical units, the eccentricity is 0.062-0.574, and the inclination is 2.2 °～ fifty-two point one °， Asteroids are 0.3-38.5 km in diameter, and more than 70 such asteroids have been found. The orbit characteristics of Apollo asteroids are that the perihelion distance is less than 1.017 astronomical units, and the half major diameter is more than 1 astronomical unit. Because there is a section of orbit which is very close to or even intersects with the earth's orbit, astronomers pay special attention to it. More than 100 such asteroids have been found. Arden type asteroids are less than 1 astronomical unit in orbit, perihelion distance is less than 1 astronomical unit, and far solar distance is slightly more than 1 astronomical unit. There are only about 10 such asteroids. Because their orbits are similar to the earth and their periods are not much different, they are paid more attention than Apollo type asteroids
the orbits of some near Earth Asteroids will intersect with the orbits of the earth under the perturbation of large planets, so they may collide with the earth. In the past few billion years, such events may have happened. Through space remote sensing technology, more than 100 craters have been found on the earth, of which 91 are presumed to be caused by asteroid impact. According to scientists' research, the parent body of JILIN METEORITE rain in 1976 was a fragment of Apollo type asteroid close to Mars orbit. Recently, scientists in the United States have suggested that the Apollo asteroid that led to the extinction of dinosaurs 65 million years ago was also a falling asteroid
although the damage caused by asteroid impact on the earth is great, the probability is very small. Research shows that asteroids with a diameter of 10 kilometers collide with the earth only once every 100 million years on average. The earth is hit by three smaller asteroids every million years, but only one of them occurs in the middle of the earth
although asteroids are very small, they have played an important role in previous astronomical studies. For example, in 1873, the German astronomer gale used the No. 8 Venus to rush to the sun, and in 1877, the British astronomer Jill used the No. 4 Vesta to rush to the sun to determine the distance between the sun and the earth, both of which obtained accurate results. From 1930 to 1931, ring the great rush of Eros 433, the International Astronomical Union organized an international joint survey on an unprecedented scale, and obtained the most accurate value of sun earth distance that can be achieved by triangulation, which is 149.58 million km< In addition, asteroids can be used to determine the mass of planets. When an asteroid approaches a major planet, the perturbation of the major planet will inevitably affect its orbit, and the actual mass of the planet can be calculated from the tiny change of its orbit. In 1870, the mass of Jupiter was 1 / 1047 of the mass of the sun, which was measured by astronomers when emfitletta approached Jupiter on the 29th. Today, astronomers still use this number. The mass of mercury, Venus, Saturn, Mars and other planets are measured by asteroids, and the measured values have a high accuracy
in order to improve and improve the accuracy of the catalogue, the International Astronomical Union (IAU) has organized more than ten observatories to conct long-term monitoring and rection of Ceres and other 10 asteroids, and obtain the accurate positions of the ecliptic and celestial equator from the actual data and known orbital elements
asteroids also provide important clues for the study of the origin and evolution of the solar system. According to the modern theory of the formation of the solar system, the solar system was formed by a cluster of chaotic nebulae 4.6 billion years ago. However, the specific process of the formation of the solar system by nebulae can no longer be traced from the earth or other planets. Only asteroids and comets still retain many of the early states of the solar system, so they are called "living fossils" of the early solar system by astronomers
in addition, asteroid research is of great significance for the development of human space instry, the protection of the earth's environment and the development of the universe. In particular, near Earth Asteroids, which are not only potential mineral resources, but also the most easily realized target of space exploration among asteroids
the diameter of asteroids is very small. In the radius values of hundreds of asteroids obtained by astronomers, only a few larger and closer asteroids are measured directly, and the others are measured by infrared wave and polarization method. Measurements show that there are about 110 asteroids with a diameter of more than 100 km, and about 560 asteroids with a diameter of more than 50 km. Most of the asteroids have a diameter of 1-2 km, which is not as big as a mountain on earth
as for the mass of asteroids, except Ceres No.1, Ares No.2 and Vesta No.4, the mass of all asteroids is calculated by their diameter and assumed density, and only the concept of order of magnitude. It is generally believed that the total mass of asteroids is 100 billion tons, of which Ceres accounts for about half of the total mass
the albedo of asteroids depends on their chemical composition and surface conditions. Because of the different albedo of each part of the asteroid surface and its rotation, the brightness of the asteroid changes periodically. According to the brightness curve, the rotation period and the orientation of the rotation axis of asteroids can be measured, and their shapes can be inferred. Judging from more than 200 known asteroids, most of them have rotation periods of 4-16 hours, with an average of 11.47 hours. The orientation of the rotation axis is randomly distributed. Asteroids larger than 100 km in diameter are generally regular in shape, close to spherical, while asteroids smaller than 100 km in diameter are various in shape, some are long cylindrical, some are like mbbells, and some are even like two stones stuck together
since the end of 1950s, the Zijinshan Observatory in China has published dozens of asteroid luminosity curves, some of which were first published in the world. Due to the high observation quality, they have been widely used by foreign observers< On October 29, 1991, the Galileo spacecraft passed the 951 asteroid gaspa and approached the asteroid at a distance of 1600 km. The detailed features of the asteroid's surface of 50 meters can be clearly seen. Preliminary measurements by the near-infrared mapping spectrometer on board the spacecraft show that Gaspar's shape is very irregular and may have been split from a large matrix. This is the first asteroid detected by the spacecraft< In August 1993, Galileo flew by 243 IDA, making it the second asteroid visited by a spacecraft. Gaspra and Ida are both metal rich and belong to S-type asteroids< On June 27, 1997, near and 253 Mathilde passed by. This is the first time that scientists have been able to observe the carbon rich C-type asteroid at close range. This visit is the only one because near detector is not specially used to investigate it. Near was used to investigate Eros asteroid in January 1999
many asteroids have been observed on the ground by astronomers. Some famous asteroids include toutais, Castalia, Vesta and geographes. For the asteroids touratis, Castalia and geographes, astronomers study them on the ground through radio observations when they approach the sun. Vesta was discovered by the Hubble Space Telescope. At present, Italy has developed a space exploration program for near Earth Asteroids named Piazzi, preparing to explore Eros near earth< On June 7, 1978, American astronomer McMahon discovered a satellite named 1978 (532) I when he observed 532 Hercules to cover its star. This is the first time that astronomers have discovered an asteroid with a satellite. Asteroid 532 and its satellite are 243 km and 45.6 km in diameter, 977 km apart from each other. Half a year later, astronomers discovered that there are satellites in Yushen star 18 from the data of its star covering. The center distance of the two small objects is 460 km, and the diameter is 135 km and 37 km respectively. If this is a synchronous satellite, the angular diameter of the "Moon" on Yushen star can reach 5 ° Its apparent area is almost 120 times that of our moon. Later, when reprocessing the occultation data of some asteroids in the past, it was found that a number of asteroids also had satellites, including Zhishen No. 2, Chunshen No. 6, Haishen No. 9 and kaishen No. 12, with about 30 to 40 satellites< In 1980, U.S. astronomers used the new technology of spot interferometry to prove that there was indeed a satellite in Zhishen 2. However, the issue of whether there was a satellite in asteroid remains unresolved. Some astronomers who hold opposing opinions believe that human beings have launched so many space probes, but so far no asteroid satellite has been found, So the conclusion that asteroids have satellites lacks observational evidence. In addition, there is no final conclusion about the level of asteroid satellites in the celestial system and whether they can be compared with the moon or Ganymede< In October 1991, Galileo, the Jupiter probe launched in 1989, flew past Gaspar, the 951 asteroid, fulfilling Astronomers' dream of exploring asteroids. In August 1993, "Galileo" swept over IDA, the No. 243 asteroid, and made a number of observations. In February 1994, astronomers analyzed the data sent back by Galileo and found that there was a much smaller satellite near IDA. They published a group photo of IDA and the satellite and a magnified image of the satellite in the British academic weekly nature. Since then, Galileo has sent back updated imaging and spectral data. According to this, astronomers estimated that the diameter of IDA satellite was 1.5 km, and the discovery time was only 100 km away from the asteroid. Astronomers believe that this is the first case of the discovery of an asteroid with a satellite<
the orbital distribution of asteroids
the orbits of asteroids are oval, about 95% of the asteroids' orbits are between 2.17 and 3.64 astronomical units. This space area is called the main belt of asteroids, and the asteroids in the main belt are called "main belt asteroids"
a small number of asteroids are isolated and form several special groups. Distant asteroids with orbital radii greater than 3.3 astronomical units are called distant asteroids. Among them, the most famous is the Toro central group, whose orbital radii are as large as those of Jupiter. From the sun, there are some 60 years ahead of Jupiter °， Some are 60 years behind Jupiter °， The former is called "Greek group", and the latter is called "pure Toro central group"
another special group is near Earth Asteroids, whose orbit perihelions go deep into the inner solar system, and some even run into the earth's orbit, which is called near Earth Asteroids. According to the numerical characteristics of the distance and half major diameter of the orbit perihelion, the near earth asteroids are divided into amore type, Apollo type and Arden type
the orbital characteristics of amore asteroids are that the perihelion is within the orbit of Mars - 1.02-1.3 astronomical units, the half major diameter is 1.39-4.23 astronomical units, the eccentricity is 0.062-0.574, and the inclination is 2.2 °～ fifty-two point one °， Asteroids are 0.3-38.5 km in diameter, and more than 70 such asteroids have been found. The orbit characteristics of Apollo asteroids are that the perihelion distance is less than 1.017 astronomical units, and the half major diameter is more than 1 astronomical unit. Because there is a section of orbit which is very close to or even intersects with the earth's orbit, astronomers pay special attention to it. More than 100 such asteroids have been found. Arden type asteroids are less than 1 astronomical unit in orbit, perihelion distance is less than 1 astronomical unit, and far solar distance is slightly more than 1 astronomical unit. There are only about 10 such asteroids. Because their orbits are similar to the earth and their periods are not much different, they are paid more attention than Apollo type asteroids
the orbits of some near Earth Asteroids will intersect with the orbits of the earth under the perturbation of large planets, so they may collide with the earth. In the past few billion years, such events may have happened. Through space remote sensing technology, more than 100 craters have been found on the earth, of which 91 are presumed to be caused by asteroid impact. According to scientists' research, the parent body of JILIN METEORITE rain in 1976 was a fragment of Apollo type asteroid close to Mars orbit. Recently, scientists in the United States have suggested that the Apollo asteroid that led to the extinction of dinosaurs 65 million years ago was also a falling asteroid
although the damage caused by asteroid impact on the earth is great, the probability is very small. Research shows that asteroids with a diameter of 10 kilometers collide with the earth only once every 100 million years on average. The earth is hit by three smaller asteroids every million years, but only one of them occurs in the middle of the earth
6. The top floor of Shanghai Center Tower has not been opened to tourists for the time being. Only 118 floors of sightseeing hall have been opened.
7. Modes that can improve proficiency:
in fact, whether playing games with players or with computers, in the king's glory, as long as the game team (the number of players is equal), it can gain experience, and the proficiency of man-machine and actual combat can be obtained<
how to brush the king's glory proficiency
limited time activity is a good choice:
there are some modes, a game can be played quickly, such as the battle of Flame Mountain, which gives a lot of proficiency. When it's open time, you might as well call several friends who have experience in this mode to play together<
how to brush the king's glory proficiency 2
the success or failure determines the proficiency level:
is it that as long as you play games, the proficiency will rise very fast? It's not that the result of the game, whether you win or lose, is directly related to your operation and your kDa score<
how to brush the king's glory proficiency 3
you can see the Proficiency Badge in the hero list:
we can see our hero's proficiency in our hero list and in the loading interface of our game. Different proficiency has different color badges to show us, such as blue and purple<
how to brush the king's glory proficiency 4
click the hero to see the specific value:
if you want to see the hero's specific proficiency and when it can be upgraded, you might as well check the hero. Click the hero and you will have the specific proficiency value when you have time. It's very clear<
how to brush the king's glory proficiency 5
each game record will show the increased value:
after each game, there will be a judgment interface for how many gold coins and experience will be increased. In this interface, we can also see the increased proficiency of heroes
runes can help us improve the winning rate:
in order to improve our proficiency faster, we must ensure that our game can win. In addition to more practice, we should speed up the time to upgrade and extract the appropriate runes, which can make you win more guaranteed.
in fact, whether playing games with players or with computers, in the king's glory, as long as the game team (the number of players is equal), it can gain experience, and the proficiency of man-machine and actual combat can be obtained<
how to brush the king's glory proficiency
limited time activity is a good choice:
there are some modes, a game can be played quickly, such as the battle of Flame Mountain, which gives a lot of proficiency. When it's open time, you might as well call several friends who have experience in this mode to play together<
how to brush the king's glory proficiency 2
the success or failure determines the proficiency level:
is it that as long as you play games, the proficiency will rise very fast? It's not that the result of the game, whether you win or lose, is directly related to your operation and your kDa score<
how to brush the king's glory proficiency 3
you can see the Proficiency Badge in the hero list:
we can see our hero's proficiency in our hero list and in the loading interface of our game. Different proficiency has different color badges to show us, such as blue and purple<
how to brush the king's glory proficiency 4
click the hero to see the specific value:
if you want to see the hero's specific proficiency and when it can be upgraded, you might as well check the hero. Click the hero and you will have the specific proficiency value when you have time. It's very clear<
how to brush the king's glory proficiency 5
each game record will show the increased value:
after each game, there will be a judgment interface for how many gold coins and experience will be increased. In this interface, we can also see the increased proficiency of heroes
runes can help us improve the winning rate:
in order to improve our proficiency faster, we must ensure that our game can win. In addition to more practice, we should speed up the time to upgrade and extract the appropriate runes, which can make you win more guaranteed.
8. Subway line 2
Lujiazui Station
Exit 6
is just in front of you
Lujiazui Station
Exit 6
is just in front of you
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