✦ LIBER ✦

Explosive events, magnetic reconnection, and coronal heating

✍ Scribed by K.P. Dere

Publisher: Elsevier Science
Year: 1994
Tongue: English
Weight: 713 KB
Volume: 14
Category: Article
ISSN: 0273-1177
DOI: 10.1016/0273-1177(94)90154-6

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Magnetic reconnection: flares and corona

Magnetic reconnection: flares and coronal heating in active galactic nuclei

✍ T. Di Matteo 📂 Article 📅 1998 🏛 John Wiley and Sons 🌐 English ⚖ 318 KB

Preliminary observations of coronal magn

Preliminary observations of coronal magnetic fields before and after solar proton events

✍ Jesusa Valdez; Martin D. Altschuler 📂 Article 📅 1970 🏛 Springer 🌐 English ⚖ 361 KB

Maps of the coronal magnetic field before and after several proton flares were examined. There are indications that large scale changes occur in both the photospheric and coronal magnetic field as a consequence of large proton flares.

Proof-of-principle experiment on control

Proof-of-principle experiment on control of ion flow and ion heating during magnetic reconnection

✍ Yukihiro Murata; Yasushi Ono 📂 Article 📅 2004 🏛 John Wiley and Sons 🌐 English ⚖ 923 KB

Heating and reconnection of the emerging

Heating and reconnection of the emerging magnetic flux-tubes and the role of the interchange instability

✍ Yutaka Uchida; Takashi Sakurai 📂 Article 📅 1977 🏛 Springer 🌐 English ⚖ 855 KB

A study of a macro-spicule and a transit

A study of a macro-spicule and a transition region explosive event in a solar coronal hole

✍ M.D. Popescu; L.D. Xia; D. Banerjee; J.G. Doyle 📂 Article 📅 2007 🏛 Elsevier Science 🌐 English ⚖ 811 KB

Observations of preburst heating and mag

Observations of preburst heating and magnetic field changes in a coronal loop at 20 cm wavelength

✍ Robert F. Willson 📂 Article 📅 1984 🏛 Springer 🌐 English ⚖ 731 KB

The Very Large Array (VLA) has been used at 20 cm wavelength to study the evolution of a burst loop with 4" resolution on timescales as short as 10 s. The VLA observations show that the coronal loop began to heat up and change its structure about 15 rain betbre the eruption of two impulsive bursts.