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20022022
most citedLimb Spicules from the Ground and from Space

56 citations · 368 across the 20 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 15 cited

The X-Ray Environment During the Epoch of Terrestrial Planet Formation: Chandra Observations of h Persei

Thayne Currie, Nancy Remage Evans, Brad Spitzbart +5

We describe Chandra/ACIS-I observations of the massive ~ 13--14 Myr-old cluster, h Persei, part of the famous Double Cluster (h and chi Persei) in Perseus. Combining the list of Ch…

astro-ph2007★ 21 cited

Galactic Edge Clouds I: Molecular Line Observations and Chemical Modelling of Edge Cloud 2

P. M. E. Ruffle, T. J. Millar, H. Roberts +5

Edge Cloud 2 (EC2) is a molecular cloud, about 35 pc in size, with one of the largest galactocentric distances known to exist in the Milky Way. We present observations of a peak CO…

astro-ph2006★ 42 cited

Charon's radius and density from the combined data sets of the 2005 July 11 occultation

M. J. Person, J. L. Elliot, A. A. S. Gulbis +4

The 2005 July 11 C313.2 stellar occultation by Charon was observed by three separate research groups, including our own, at observatories throughout South America. Here, the publis…

astro-ph2005★ 18 cited

The Effect of the Transit of Venus on ACRIM's Total Solar Irradiance Measurements: Implications for Transit Studies of Extrasolar Planets

G. Schneider, J. M. Pasachoff, R. C. Willson

We used the 8 June 2004 transit of Venus (ToV) as a surrogate to test observing methods, strategies and techniques that are being contemplated for future space missions to detect a…

astro-ph2003

Space Studies of the Black-Drop Effect at a Mercury Transit

G. Schneider, J. M. Pasachoff, L. Golub

Transits of Mercury and Venus across the face of the Sun are rare. The 20th century had 15 transits of Mercury and the 21st century will have 14, the two most recent occuring on 15…

astro-ph2002★ 31 cited

Short-Period Waves That Heat the Corona Detected at the 1999 Eclipse

Jay M. Pasachoff, Bryce A. Babcock, Kevin D. Russell +1

As a part of a study of the cause of solar coronal heating, we searched for high-frequency (~1 Hz) intensity oscillations in coronal loops in the [Fe XIV] coronal green line. We su…