Bridge, H. S.; Belcher, J. W.; Coppi, B.; Lazarus, A. J.; McNutt Jr., R. L.; Olbert, S.; Richardson, J. D.; Sands, M. R.; Selesnick, R. S.; Sullivan, J. D.et al.; Hartle, R. F.; Ogilvie, K. W.; Sittler Jr., E. C.; Bagenal, F.; Wolff, R. S.; Vasyliūnas, V. M.; Siscoe, G. L.; Goertz, C. K.; Eviatar, A.: Plasma observations near Uranus: Initial results from Voyager 2. Science 233, pp. 89 - 93 (1986)
Goertz, C. K.; Nielsen, E.; Korth, A.; Glassmeier, K. H.; Haldoupis, C.; Hoeg, P.; Hayward, D.: Observations of a possible ground signature of flux-transfer events. Journal Geophysical Research 90, p. 4069 (1985)
Bridge, H. S.; Bagenal, F.; Belcher, J. W.; Lazarus, A. J.; McNutt, R. L.; Sullivan, J. D.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 2. Science 215, pp. 563 - 570 (1982)
Marsch, E.; Goertz, C. K.; Richter, K.: Wave heating and acceleration of solar wind ions by cyclotron resonance. Journal Geophysical Research 87, pp. 5030 - 5044 (1982)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Olbert, S.; Sullivan, J. D.; Bagenal, F.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 1. Science 212, pp. 217 - 224 (1981)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Sullivan, J. D.; Bagenal, F.; McNutt Jr., R. L.; Ogilvie, K. W.; Scudder, J. D.; Sittler, E. C.; Vasyliūnas, V. M.et al.; Goertz, C. K.: Plasma observations near Jupiter: Initial results from Voyager 2. Science 206, pp. 972 - 976 (1979)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Sullivan, J. D.; McNutt, R. L.; Bagenal, F.; Scudder, J. D.; Sittler, E. C.; Siscoe, G. L.; Vasyliūnas, V. M.et al.; Goertz, C. K.; Yeates, C. M.: Plasma observations near Jupiter: Initial results from Voyager 1. Science 204, pp. 987 - 991 (1979)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.