Fayl:Solar-filament.gif
Navigatsiya qismiga oʻtish
Qidirish qismiga oʻtish
Bundan kattaroq tasvir yoʻq.
Solar-filament.gif (669 × 478 piksel, fayl hajmi: 114 KB, MIME tipi: image/gif)
Qisqa izoh
| Taʼrif |
English: Filament erupting during a solar flare, seen at EUV wavelengths that show both emission and absorption (the filament has both).
The plasma physics involved in this process remains ill-understood, but it certainly involves the Sun's magnetic field. Picture Credit: TRACE, NASA. Source |
| Manba | NASA |
| Muallif | NASA |
Litsenziyalash
|
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
 |
Warnings:
|
Original upload log
The original description page was here. All following user names refer to en.wikipedia.
- 2005-10-04 10:06 Iantresman 669×478×6 (116850 bytes) Filaments surrounding a solar flare, caused by the interaction of the [[plasma]] in the Sun's atmopshere with its magnetic field. Picture Credit: TRACE, NASA. [http://antwrp.gsfc.nasa.gov/apod/ap040725.html Source]
Fayl tarixi
Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.
| Sana/Vaqt | Miniatura | Oʻlchamlari | Foydalanuvchi | Izoh | |
|---|---|---|---|---|---|
| joriy | 10:19, 2008-yil 17-iyun | | 669 × 478 (114 KB) | wikimediacommons>Sir48 | {{Information |Description={{en|Filament erupting during a solar flare, seen at EUV wavelengths that show both emission and absorption (the filament has both). The plasma physics involved in this process re |
Fayllarga ishoratlar
Bu faylga quyidagi sahifa bogʻlangan:
