gong.nso.edu

sol-uruguay-sol.blogspot.com

Sol - Uruguay - Sol: octubre 2014

http://sol-uruguay-sol.blogspot.com/2014_10_01_archive.html

Lunes, 27 de octubre de 2014. Trabajos de estudiantes de la Scuola Italiana (Prof.M. Martinez). Fotografías tomada por estudiantes demostrando la rotación solar. La mancha gigante tomada desde la Scuola por estudiante. Observatorio Liceo 58 (Prof. R.Salvo). Enviar por correo electrónico. Sábado, 25 de octubre de 2014. La Mancha Gigante desde el Observatorio Guyunusa: Liceo 65 (Prof. F.Albornoz). Observatorio Liceo 58 (Prof. R.Salvo). Enviar por correo electrónico. Viernes, 24 de octubre de 2014. Enorme m...

nisp.nso.edu

NISP News | NISP

http://nisp.nso.edu/news

June 17, 2014. NSO joins in International Sun Day. May 8, 2014. An X-Class Flare at High Resolution. March 11, 2014. In Memoriam - Irene González Hernández. February 24, 2014. 2014 AURA Awards Announced. February 13, 2014. January 16, 2014. Fickle Fields: Are Transient Magnetic Reversals Real? January 9, 2014. Ground-based Telescopes Observe Largest Solar Flare of 2014. December 3, 2013. Putting Uncertainties to Space Weather Forecast. July 10, 2013. SOLIS Observations Give New Insights into Space Weather.

nisp.nso.edu

Solar Interior | NISP

http://nisp.nso.edu/solar_interior

Located around the world. Continue Reading on Solar Interior. Submitted by Kiran Jain. On Thu, 09/17/2015 - 12:58. NSO Integrated Synoptic Program. The National Solar Observatory is operated by the Association of Universities for Research in Astronomy under a cooperative agreement with the National Science Foundation, for the benefit of the astronomical community.

nisp.nso.edu

About GONG | NISP

http://nisp.nso.edu/aboutgong

The Global Oscillation Network Group (GONG) is a community-based project to conduct a detailed study of solar internal structure and dynamics using helioseismology. A major challenge in helioseismology is uncertainties and errors imposed by day-night cycles and local observatory weather. Overcoming single observatory limitations, GONG has deployed a network of six inexpensive instruments around the world to provide nearly continuous, extremely sensitive, observations of the solar velocities.

la1tna.net

SOLARCYCLE 24 - www.la1tna.net

http://www.la1tna.net/20955001

VIDEO CLIP no 1. Video Clip no 2. VIDEO CLIP no 3. VIDEO CLIP no 4. VIDEO CLIP no 5. Cycle 24 Records (Since Jan 2008). SOLAR Flux - 190. FLARE - X6.9. Geomagnetic A Indice - -. DAYS IN A ROW WITH A SUNSPOT - 198. Latest Solar News and Updates. CME Update / Solar Update. 2/24/2012 by Kevin VE3EN at 21:10 UTC. Comment on Message Board. Updated 2/24/2012 @ 21:10 UTC. Coronal Mass Ejection Part II and III. To watch the latest model run. Updated 2/24/2012 @ 14:20 UTC. Added 2/23/2012 @ 11:50 UTC. A Coronal M...

nisp.nso.edu

Solar Atmosphere | NISP

http://nisp.nso.edu/solar_atmosphere

Research conducted in the framework of the Solar Atmosphere group of the NSO Integrated Synoptic Program (NISP) is aimed at understanding and forecasting the solar activity cycle, the evolution and topology of solar magnetic fields, the physics of solar active phenomena (flares and CMEs), the solar irradiance changes and their relationship to global change. The group is also involved in studies pertinent to solar-stellar and sun-as-a-star research. Continue Reading on Solar Atmosphere.

nisp.nso.edu

Space Weather | NISP

http://nisp.nso.edu/space_weather

One of the first objects that Galileo looked at through his telescope was the Sun, where he quickly noticed the presence of dark areas that are known as sunspots. Sometime later, it was noticed that the number of sunspots seemed to rise and fall with a period of about 11 years, marking the discovery of the sunspot or solar activity cycle. Aurorae observed from space on Jupitor (left), Earth (Center), and Saturn (Right). Continue Reading on Space Weather . On Mon, 03/31/2014 - 13:48.

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...

nisp.nso.edu

About SOLIS | NISP

http://nisp.nso.edu/aboutsolis

Synoptic Optical Long-term Investigations of the Sun. SOLIS is composed of a single equatorial mount (right) carrying three telescopes:. 50 cm Vector Spectromagnetograph (VSM). 14 cm Full-Disk Patrol (FDP). 8 mm Integrated Sunlight Spectrometer (ISS). On Mon, 03/31/2014 - 09:12. NSO Integrated Synoptic Program.

sdo3.lws-sdo-workshops.org

LWS/SDO-3/SOHO-26/GONG-2011 Workshop - Home

http://sdo3.lws-sdo-workshops.org/index.php

Skip to main navigation. Skip to first column. Skip to second column. Solar Dynamics and Magnetism from the Interior to the Atmosphere. October 31-November 4, 2011. Are now available ( Late Abstracts. Please, sign up for Mini-Workshops and Technical Meetings. Sign up for the NASA Ames Tour. Now available only for US citizens and permanent residents). Travel and Parking Information. Workshop webcast: http:/ www.livestream.com/bccconferencechannel. NASA's Solar Dynamics Observatory. The data is being used ...