Fichier:Solar Eruption.jpg
Ñatanaʋ pʋnɛ pɩ-walanzɩ : Kpaɣna pɩkɩsɛlɩ 600 nɛ pɩtalɩ 600 ñɩŋgʋ. Tʋtʋ lɛɛtʋ : Kpaɣna pɩkɩsɛlɩ 240 nɛ pɩtalɩ 240 ñɩŋgʋ | Kpaɣna pɩkɩsɛlɩ 480 nɛ pɩtalɩ 480 ñɩŋgʋ | Kpaɣna pɩkɩsɛlɩ 768 nɛ pɩtalɩ 768 ñɩŋgʋ | Kpaɣna pɩkɩsɛlɩ 1 200 nɛ pɩtalɩ 1 200 ñɩŋgʋ.
Kiɖe tɛɛ takayaɣ (Kpaɣna pɩkɩsɛlɩ 1 200 nɛ pɩtalɩ 1 200 ñɩŋgʋ, takayaɣ walanzɩ : 596 kio, MIME akɩlɩ : image/jpeg)
Kɛdɩtʋ
| Kɛdɩtʋ |
English: A solar eruption gracefully rose up from the sun on Dec. 31, 2012, twisting and turning. Magnetic forces drove the flow of plasma, but without sufficient force to overcome the sun’s gravity much of the plasma fell back into the sun.
The length of the eruption extends about 160,000 miles out from the Sun. With Earth about 7,900 miles in diameter, this relatively minor eruption is about 20 times the diameter of our planet. |
||
| Efemiye |
|
||
| Kiɖe | http://www.nasa.gov/multimedia/imagegallery/image_feature_2422.html | ||
| Mayʋ | NASA/SDO |
Labɩnaʋ paɣtʋ
|
Ce fichier provient de la NASA. Sauf exception, les documents créés par la NASA ne sont pas soumis à copyright. Pour plus d'informations, voir la politique de copyright de la NASA. |  |
 |
Attention :
|
Takayaɣ caanaʋ tɔm kɛdʋʋ
Tukina efemiye nɛ ñɩɣtʋ nɛ ŋna takayaɣ kanɛ ɛzɩ kaawɛʋ alɩwaatʋ ndʋ tɩ-taa yɔ.
| Efemiye nɛ ñɩɣtʋ | Tampɔɔ | Walanzɩ | Labɩnayʋ | Tɔm taa nuutuu | |
|---|---|---|---|---|---|
| lɛlɛɛyɔ | 17 Kɔlaɣ fenaɣ 2013 à 05:48 | | 1 200 × 1 200 (596 kio) | Salamander724 | {{Information |Description ={{en|1=A solar eruption gracefully rose up from the sun on Dec. 31, 2012, twisting and turning. Magnetic forces drove the flow of plasma, but without sufficient force to overcome the sun’s gravity much of the plasma fel... |
Takayaɣ labɩnaʋ
Takayɩhayʋʋ kɩtɩŋʋʋ lakɩna takayaɣ kanɛ tʋmɩyɛ :
takayaɣ labɩnaʋ nɛ paa anɩ
Wikinaa kɩtɩŋaa lɛlaa lakɩna kɩlɛmʋʋ kʋnɛ nɛ tʋmɩyɛ :
- Labɩnaʋ zh.wikibooks.org yɔɔ
