Speaker
Jakub Vaverka
(Department of Physics, Umeå University, Sweden)
Description
There are several different techniques that are used to measure cosmic dust entering
the Earth's atmosphere such as space-born dust detectors, meteor and HPLA radars, and
optical methods. One complementary method could be to use electric field instruments
initially designed to measure electric waves. A plasma cloud generated by a
hypervelocity dust impact on a spacecraft body can be detected by the electric field
instruments commonly operated on the spacecraft. Since Earth-orbiting missions are
generally not equipped with conventional dust detectors, the electric field
instruments offer an alternative method to measure the Earth's dust environment.
We present the first detection of dust impacts on one of the Earth-orbiting Cluster
satellites by the Wide-Band Data (WBD) instrument. We describe the concept of dust
impact detection focused on specifics of the Cluster spacecraft and the WBD
instrument. We estimate the size and the velocity of the impinging dust grains from
the amplitude of the Cluster voltage pulses and discuss sensitivity of this method
for dust grain detection.
Primary author
Jakub Vaverka
(Department of Physics, Umeå University, Sweden)
Co-authors
Alexandre De Spiegeleer
(Department of Physics, Umeå University, Sweden)
Asta Pellinen-Wannberg
(Department of Physics, Umeå University, Sweden - Swedish Institute of Space Physics, Kiruna, Sweden)
Carol Norberg
(Department of Physics, Umeå University, Sweden - Swedish Institute of Space Physics, Kiruna, Sweden)
Ingrid Mann
(Department of Physics, Umeå University, Sweden - EISCAT Scientific Association, Kiruna, Sweden)
Johan Kero
(Swedish Institute of Space Physics, Kiruna, Sweden)
Maria Hamrin
(Department of Physics, Umeå University, Sweden)
Timo Pitkänen
(Department of Physics, Umeå University, Sweden)