Area variation with temperature of supergranule network features in the solar transition zone

✍ Scribed by Edward J. Eadon; Donald E. Billings

• Publisher: Springer
• Year: 1978
• Tongue: English
• Weight: 206 KB
• Volume: 58
• Category: Article
• ISSN: 0038-0938
• DOI: 10.1007/bf00152552

✦ Synopsis

Areas of network emission features in C II )t 1135, C III A977, O IV A544 and O vIA 1032

were measured in and out of coronal holes. In the quiet Sun these areas, on the average, showed a 20% increase between C II and O vI. In the coronal holes there was no significant average variation, but a number of the features showed an interesting decrease in area at intermediate temperatures.