solarscience.msfc.nasa.gov
NASA/Marshall Solar Physics
http://solarscience.msfc.nasa.gov/corona.shtml
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Click on image for larger version. The Corona is the Sun's outer atmosphere. It is visible during total eclipses of the Sun as a pearly white crown surrounding the Sun. The corona displays a variety of features. However, during the few fleeting minutes of totality few, if any, changes are seen in these coronal features. The Emission Line Corona. The LASCO...
solarscience.msfc.nasa.gov
NASA/Marshall Solar Physics
http://solarscience.msfc.nasa.gov/CMEs.shtml
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Coronal mass ejections (or CMEs) are huge bubbles of gas threaded with magnetic field lines that are ejected from the Sun over the course of several hours. Although the Sun's corona. Coronagraph on the Solar Maximum Mission. In April of 1980. Click on image for animation. On the Solar and Heliospheric Observatory ( SOHO. Eruptions but they can also occur ...
magnetograph.msfc.nasa.gov
NASA/Marshall Solar Physics
http://magnetograph.msfc.nasa.gov/outreach/girlscouts/index.html
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Eclipses and the Sun and LEONIDS. Links to Webpages for Girl Scouts. And Frequently Asked Questions. But now includes information on observing meteor showers and learning about space weather. Observations of a meteor shower are the core of requirements for earning a Meteors and Meteor Showers. Html) and click here. For a printable pdf version. Pick out a ...
magnetograph.msfc.nasa.gov
NASA/MSFC Magnetograph
http://magnetograph.msfc.nasa.gov/index.html
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Click on image for larger version. The Marshall Space Flight Center Vector Magnetograph Facility was assembled in 1973 to support the Skylab mission. And its role in processes such as solar flares. Images from this telescope provide a view of chromospheric structures. Click for larger version. In the fall of 2005 the instrument was moved to its current lo...
ru.wikipedia.org
Гелиосфера — Википедия
https://ru.wikipedia.org/wiki/Гелиосфера
Материал из Википедии свободной энциклопедии. 160; область околосолнечного пространства, в которой плазма солнечного ветра. Извне гелиосфера ограничена бесстолкновительной ударной волной. Возникающей в солнечном ветре из-за его взаимодействия с межзвёздной плазмой. И межзвёздным магнитным полем. Первые 10 миллиардов километров скорость солнечного ветра. Составляет около миллиона километров в час. По мере того, как он сталкивается с межзвёздной средой. Источник не указан 1809 дней. Переносимое солнечным в...
solarscience.msfc.nasa.gov
NASA/Marshall Solar Physics
http://solarscience.msfc.nasa.gov/papers.shtml
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Listed alphabetically by first author. Alexander, D., Gary, G. A., and Thompson, B.J., 1998, Analysis of Active Regions via 3D Rendering Techniques'. In Proc. 2nd Advances in Solar Physics Euroconference (ASPE), Three-Dimensional Structure of Solar Active Regions, (eds. C. Alissandrakis and B. Schmieder), PASP Conference Series 155. Falconer, D.A....Falco...
solarscience.msfc.nasa.gov
NASA/Marshall Solar Physics
http://solarscience.msfc.nasa.gov/Skylab.shtml
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Click on image for larger version. The first US space station, was launched into orbit on May 14, 1973 as part of the Apollo program. This 91 metric ton structure was 36 meters (four stories) high, 6.7 meters in diameter and flew at an altitude of 435 km (270 miles). Three different Apollo crews manned. Click on image for larger version. Are seen as dark ...
magaxp1.msfc.nasa.gov
NASA/MSFC Magnetograph
http://magaxp1.msfc.nasa.gov/index.html
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). Click on image for larger version. The Marshall Space Flight Center Vector Magnetograph Facility was assembled in 1973 to support the Skylab mission. And its role in processes such as solar flares. Images from this telescope provide a view of chromospheric structures. Click for larger version. In the fall of 2005 the instrument was moved to its current lo...
magaxp1.msfc.nasa.gov
NASA/MSFC Magnetograph
http://magaxp1.msfc.nasa.gov/outreach/education/index.html
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). The Sun Has Spots! Background Information for Middle and High School Teachers:. No one here on Earth thinks a pimple on a face is cool but scientists think a spot on the Sun is very. Cool almost 2000 degrees cooler than surrounding gases which make up the surface, or photosphere, of the Sun! What is a sunspot? Finally in April of 1612, Galileo, with the h...
magnetograph.msfc.nasa.gov
NASA/MSFC Magnetograph
http://magnetograph.msfc.nasa.gov/outreach/education/index.html
The Sun in Time. Why We Study the Sun. Magnetism - The Key. THE SUN IN ACTION. Surface and Interior Flows. THE MSFC SOLAR GROUP. The Sun in Time (EPO). The Sun Has Spots! Background Information for Middle and High School Teachers:. No one here on Earth thinks a pimple on a face is cool but scientists think a spot on the Sun is very. Cool almost 2000 degrees cooler than surrounding gases which make up the surface, or photosphere, of the Sun! What is a sunspot? Finally in April of 1612, Galileo, with the h...