O Engvold
Biographic Data
| ID | 10218172 |
|---|---|
| NAME | O Engvold |
| FAMILY NAME | O Engvold |
| SIGNATURE | ENGVOLD O |
| AFFILIATIONS | Centre National de la Recherche Scientifique |
| ORCID | 0000-0001-8468-2931 |
| VERIFIED | Yes |
| TOTAL WORKS | 1 |
| TOTAL CITATIONS | 0 |
| WORKS AS AUTHOR | 1 |
| WORKS AS EDITOR | 0 |
| FIRST PUBLICATION YEAR | 2024 |
| LATEST PUBLICATION YEAR | 2024 |
| H-INDEX | 0 |
The Role of Prominences in the History of Solar Physics
The very outer solar atmosphere (corona) is very hot with temperatures over a million degrees K, while the photosphere is of the order of 5000 K. Embedded in this hot outer corona are cool, QUOTE ≤ 10,000 K, magnetic structures called solar prominences. As seen on the disk, they are long filamentary structures while on the solar limb they look like intricate loops. In this paper, we present the development of our understanding of solar prominence…
No prominent works on this page.
The Role of Prominences in the History of Solar Physics
The very outer solar atmosphere (corona) is very hot with temperatures over a million degrees K, while the photosphere is of the order of 5000 K. Embedded in this hot outer corona are cool, QUOTE ≤ 10,000 K, magnetic structures called solar prominences. As seen on the disk, they are long filamentary structures while on the solar limb they look like intricate loops. In this paper, we present the development of our understanding of solar prominence…
Astro and Planetary Science (1 work) · Astrobiology (1 work) · Astronomy (1 work) · Astrophysics (1 work) · Chromosphere (1 work) · Coronal loop (1 work) · Coronal mass ejection (1 work) · Coronal radiative losses (1 work) · Magnetic field (1 work) · Nanoflares (1 work)