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Solar thunder from SPACE … NASA research moon passes in front of the sun In interesting photos the moon of the moon is returned by the fire of the sun.
- The NASA spacecraft took the moon from space in an exciting series of photographs in front of the sun.
- The eclipse was not visible from the ground and lasted only 3 minutes, but was captured on camera from space.
- Nearby images by Solar Dynamic Observer show a range of solar mountains reflected by solar flares.
- The Leibniz and Dorfel ranges near the Moon’s South Pole have been identified by NASA experts.
Announcement
NASA satellites have taken interesting pictures of a partial solar eclipse from its unique location in space – the only place where it could be seen.
The Solar Dynamics Observer (SDO) took a picture of the moon passing over the sun yesterday at 05:20 BST (01:20 ET).
The transition lasted about 35 minutes and at its peak, the moon covered 67 percent of the flames.
The spacecraft then returned a series of photos of the incident to Space Weather. com According to experts, ‘the mountains of the moon have been illuminated by solar fire’.
Ponds and chaos can be seen on the surface of the moon passing through what is known as part of the Leibniz and Dorfel mountain ranges.
NASA’s Solar Dynamic Observer took pictures of a 35-minute-long partial solar satellite from its special place in space – the only place where it could be seen.
The Solar Dynamic Observatory took a picture of the moon in front of the sun at 05:20 BST (01:20 ET) yesterday.
According to SpaceWeather.com experts, the satellite has retrieved a series of images showing the moon’s mountains illuminated by solar flares.
Patricio Leon, from Santiago, Chile, compares near-moon images of the moon moving along the sun with a topographic map from a solar observatory.
He was able to explore the Lebanese and Dorfel mountain ranges near the moon’s south pole during Eid.
Experts at SpaceWeather.com said: ‘During the lunar thunderstorm, the moon covered 67 percent of the sun, and the moon’s mountains were illuminated by solar fire.
High-resolution images like this can help the SDO science team better understand the telescope.
‘They show how light differs around SDO feedback and filter support grades.
Once it is calibrated, it is possible to adjust the SDO data for instrumental effects and make the sun images even faster than before.
Launched in 2010, NASA’s Solar Dynamic Observer monitors the sun with a satellite spacecraft, taking pictures of it every 0.75 seconds.
It also studies the solar magnetic field, atmosphere, solar spaces and other aspects that affect performance during the 11-year solar cycle.
The Sun has been experiencing high performance for several months now as it looks like it is moving into its particularly active period of 11 years, which started in 2019 and is expected to rise in 2025.
The sun’s magnetic poles are paralyzed during a period of solar activity, and a magnetic field made up of charged particles from the solar wind travels through the surface of the sun and through the solar system.
This is accompanied by an increase in solar radiation and coronal mass ejection (CMEs) from the surface of the sun.
A CME is a significant release of plasma and joins a magnetic field from the sun’s corona – the outer part of the sun’s atmosphere – to the solar wind.
CMEs only affect the Earth when they are aimed at our planet, and They are much slower than solar rays because they move large amounts of matter.
Patricio Leon, from Santiago, Chile, compares near-moon images of the moon moving along a topographic map from a solar observation orbit he was able to identify the Leibniz and Dorfil mountain ranges near the moon’s south pole.
The Solar Dynamics Observatory (SDO), pictured here, studies how solar activity is generated and how atmospheric air results from this activity.
The energy from the beam can disrupt the area of the atmosphere through which radio waves travel, which can cause temporary blackouts in navigation and communication signals.
CMEs, on the other hand, have the power to suspend the Earth’s magnetic field, creating a flow that allows particles to move towards the Earth’s poles.
When it reacts with oxygen and nitrogen, they help form the aurora, also known as the northern and southern lights.
In addition, magnetic changes can affect a variety of human technologies, GPS coordinates can be routed by multiple yards and power grids become more frequent when the power company is not ready.
No CME or solar radiation has been seen in the modern world – the most recent being the Carrington incident in 1859 – creating a geomagnetic storm that appears around the world with aurora, as well as fires in telegraph stations.
What is NASA’s Solar Dynamic Observatory?
The Solar Dynamics Observer (SDO) is a NASA mission that has been monitoring the sun since 2010.
Its ultra-HD camera converts different wavelengths of light into images that can be seen by humans, and the light is then colored into a rainbow of colors.
The satellite was launched from Cape Canaveral on February 9, 2013.
The SDO has a set of tools that provide observations that lead to a complete understanding of the solar dynamics that cause changes in the Earth’s environment.
One of the most incredible images provided by SDO
Among the tasks this set of instruments can achieve are measuring ultraviolet light, differences in the sun’s magnetic field, taking pictures of the chromosphere and internal corona, and taking solar changes that may occur at different times in the solar system. Be available.
It does this using three separate devices: heliosismic and magnetic imaging; Atmosphere Painting Council And experience a very variable ultraviolet.
Science teams receive this information, which they reprocess, analyze, archive, and disseminate to the public.
