Borrero, J. M.; Martinez-Pillet, V.; Schlichenmaier, R.; Solanki, S. K.; Bonet, J. A.; del Toro Iniesta, J. C.; Schmidt, W.; Barthol, P.; Gandorfer, A.; Domingo, V.et al.; Knoelker, M.: Supersonic Magnetic Upflows in Granular Cells Observed with SUNRISE/IMaX. Astrophysical Journal 723 (2), pp. L144 - L148 (2010)
Borrero, J. M.; Rempel, M.; Solanki, S. K.: Spectropolarimetric analysis of 3D MHD sunspot simulations. Astron. Nachrichten 331 (6), pp. 567 - 569 (2010)
Borrero, J. M.: The structure of sunspot penumbrae - IV. MHS equilibrium for penumbral flux tubes and the origin of dark core penumbral filaments and penumbral grains. Astronomy and Astrophysics 471, pp. 967 - 975 (2007)
Borrero, J. M.; Solanki, S. K.; Lagg, A.; Socas-Navarro, H.; Lites, B.: On the fine structure of sunspot penumbrae: III. The vertical extension of penumbral filaments. Astronomy and Astrophysics 450, pp. 383 - 393 (2006)
Borrero, J. M.; Bellot Rubio, L. R.; Barklem, P. S.; Del Toro Iniesta, J. C.: Accurate atomic parameters for near-infrared spectral lines. Astronomy and Astrophysics 404, p. 749 (2003)
Bellot Rubio, L. R.; Borrero, J. M.: Iron abundance in the solar photosphere. Application of a two-component model atmosphere. Astronomy and Astrophysics 391 (3), pp. 331 - 337 (2002)
Borrero, J. M.; Rubio, L. R. B.: A two-component model of the solar photosphere from the inversion of spectral lines. Astronomy and Astrophysics 385 (3), pp. 1056 - 1072 (2002)
Borrero, J. M.; Lagg, A.; Solanki, S. K.; Frutiger, C.; Collados, M.; Bellot Rubio, L. R.: Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles. Astronomical Society of the Pacific, pp. 235 - 242 (2003)
Borrero, J. M.; Lagg, A.; Solanki, S. K.; Frutiger, C.; Collados, M.; Bellot Rubio, L. R.: Modeling the Fine Structure of a Sunspot Penumbra through the Inversion of Stokes Profiles. In: Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST, p. 235 (Eds. Pevtsov, A. A.; Uitenbroek, H.). (2003)
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
The MPS instruments on board ESA’s JUICE spacecraft have successfully completed their commissioning in space - and delivered their first observational data.
The launch was successful; the ESA’s space probe JUICE is now on its way to the Jupiter system. There, it will primarily study the gas giant's icy moons.
ESA's space probe is on the move: First it heads for the launch site in Kourou - and in April it will begin its long journey to Jupiter and its icy moons.