The Owens Valley Frequency-Agile Interferometer.

Hurford, G. J.

doi:10.21236/ada131825

Cited by 2 publications

(2 citation statements)

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“…Webb et al (1983) andSchmahl et aL (1982) agree that the peaks of brightness at 6 cm and in the XUV do not coincide, but at best, overlap. This result rules out free-free emission but gyroresonance emission is not completely satisfactory either.…”

Section: Coronal Loopsmentioning

confidence: 95%

“…Bremsstrahlung predominates in the feet and gyroresonance in the tops. The tops have the following properties: B = 130-170 G, T = 1.7 • 10 6 K, N= 5 • 108cm -3, fl= 3 • 10 -4 Hurford (1983) has developed a clever technique for determining coronal magnetic fields in active regions. Microwave spectra (1-18 GHz) change slope at locations within an active region where the gyroresonance opacity decreases abruptly, because of a rapid change with height of the magnetic field and temperature.…”

Section: Coronal Loopsmentioning

confidence: 99%

See 1 more Smart Citation

Progress in coronal physics

Zirker

1985

Sol Phys

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This paper reviews research highlights of the past five years. Considerable progress has been made in observing and interpreting coronal mass ejections. The stability of coronal loops is much better understood and new observations of the onset of wind streams in coronal holes have been made. Observations from the Solar Maximum Mission should helpt to clarify the physics of the active corona.The mechanisms that heat the corona and accelerate the high-speed wind streams remain to be identified, however. Solar Physics 100 (1985) 281-287. 0038-0938/85.15. 9 1985 by D. Reidel Publishing Company

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Section: Coronal Loopsmentioning

confidence: 95%

Section: Coronal Loopsmentioning

confidence: 99%