Five times the solar disk in a long row from left to right with main colors orange, light green, blue, green-red sprinkles, blue-to-red gradient, respresenting exemplary PMI data products after on-board analysis from left to right: continuum intensity, magnetic field strength, magnetic field inclination, magnetic field azimuth and line-of-sight velocity.

Publications of Sebastian Lorek

Journal Article (2)

1.
Journal Article
Lorek, S.; Lacerda, P.; Blum, J.: Local growth of dust- and ice-mixed aggregates as cometary building blocks in the solar nebula. Astronomy and Astrophysics 611, A18 (2018)
2.
Journal Article
Lorek, S.; Gundlach, B.; Lacerda, P.; Blum, J.: Comet formation in collapsing pebble clouds. What cometary bulk density implies for the cloud mass and dust-to-ice ratio. Astronomy and Astrophysics 587, A128 (2016)

Talk (1)

3.
Talk
Lorek, S.; Lacerda, P.; Gundlach, B.; Blum, J.: Compression of pebbles in collapsing pebble clouds. Planet Formation and Evolution, Duisburg, Germany (2016)

Poster (2)

4.
Poster
Lorek, S.; Lacerda, P.; Blum, J.: Comet formation in collapsing pebble clouds: pebble formation. American Astronomical Society, DPS meeting #48, Pasadena, USA (2016)
5.
Poster
Lorek, S.; Lacerda, P.; Gundlach, B.; Blum, J.: Size matters? Monomer radius and the transition from fractal to compact ice aggregates. 615. WE-Heraeus-Seminar "How primitive are comets?", Bad Honnef, Germany (2016)

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