Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Robert F. Willson"'
Autor:
Robert F. Willson Jr.
Publikováno v:
Names, Vol 25, Iss 3 (1977)
Externí odkaz:
https://doaj.org/article/27d7102e607d43d482f6e390f7c794d2
Publikováno v:
Anatomical sciences educationREFERENCES. 15(3)
As point-of-care ultrasound (POCUS) invades medical specialties, more students covet earlier ultrasound training programs in medical school. Determining the optimal placement and format in the curriculum remains a challenge. This study uses student p
Autor:
Robert F. Willson, Tyler D. Groff
Publikováno v:
Solar Physics. 250:89-105
Very Large Array (VLA) observations at wavelengths of 20 and 91 cm have been combined with data from the SOHO and RHESSI solar missions to study the evolution of transequatorial loops connecting active regions on the solar surface. The radio observat
Autor:
Robert F. Willson
Publikováno v:
Solar Physics. 227:311-326
Very Large Array (VLA) observations at 91-cm wavelength are combined with data from the SOHO EIT, MDI and LASCO and used to study the evolving coronal magnetic environment in which Type I noise storms and large-scale coronal loops occur. On one day,
Autor:
Robert F. Willson
Publikováno v:
Advances in Space Research. 35:1813-1821
Very Large Array (VLA) observations at 20 and 91 cm wavelength are compared with data from the SOHO (EIT and MDI) and RHESSI solar missions to investigate the evolution of decimetric Type I noise storms and Type III bursts and related magnetic activi
Autor:
Robert F. Willson
Publikováno v:
Proceedings of the International Astronomical Union. 2004:529-532
Multi-wavelength Very Large Array (VLA), SOHO and RHESSI observations have been used to study the three- dimensional structure of evolving coronal loops and related signatures of impulsive and long-lasting energy release above active regions. Here, w
Autor:
Robert F. Willson
Publikováno v:
Solar Physics. 197:399-419
Very Large Array (VLA) observations of the Sun at 91 and 400 cm wavelength have been used to investigate the radio signatures of EUV heating events and coronal mass ejections (CMEs) detected by SOHO and TRACE. Our 91 cm observations show the onset of
Publikováno v:
The Astrophysical Journal. 504:L117-L121
We present the first observations of nonthermal decimetric burst emission of the Sun using the new 400 cm (74 MHz) system at the VLA. Our VLA observations were carried out in collaboration with the Large Angle Spectroscopic Coronagraph (LASCO) and th
Autor:
Kenneth R. Lang, Robert F. Willson
Publikováno v:
Surveys in Geophysics. 19:521-555
We describe the world's largest synthesis radio telescope, the Very Large Array (VLA), and how it can be used to complement observations with the Solar and Heliospheric Observatory (SOHO) and the Yohkoh solar spacecraft. The VLA provides images with
Publikováno v:
Solar Physics. 170:299-320
The presence of coronal magnetic fields connecting active regions is inferred from decimetric observations of solar noise storms with the Very Large Array (VLA) and from soft X-ray images taken by Yohkoh. Temporal changes in the noise storms appear t