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Items: 5

1.

H2O at the Phoenix landing site.

Smith PH, Tamppari LK, Arvidson RE, Bass D, Blaney D, Boynton WV, Carswell A, Catling DC, Clark BC, Duck T, Dejong E, Fisher D, Goetz W, Gunnlaugsson HP, Hecht MH, Hipkin V, Hoffman J, Hviid SF, Keller HU, Kounaves SP, Lange CF, Lemmon MT, Madsen MB, Markiewicz WJ, Marshall J, McKay CP, Mellon MT, Ming DW, Morris RV, Pike WT, Renno N, Staufer U, Stoker C, Taylor P, Whiteway JA, Zent AP.

Science. 2009 Jul 3;325(5936):58-61. doi: 10.1126/science.1172339.

2.

Atmospheric structure and dynamics as the cause of ultraviolet markings in the clouds of Venus.

Titov DV, Taylor FW, Svedhem H, Ignatiev NI, Markiewicz WJ, Piccioni G, Drossart P.

Nature. 2008 Dec 4;456(7222):620-3. doi: 10.1038/nature07466.

PMID:
19052623
3.

Morphology and dynamics of the upper cloud layer of Venus.

Markiewicz WJ, Titov DV, Limaye SS, Keller HU, Ignatiev N, Jaumann R, Thomas N, Michalik H, Moissl R, Russo P.

Nature. 2007 Nov 29;450(7170):633-6.

PMID:
18046394
4.

Evidence from the Mars Express High Resolution Stereo Camera for a frozen sea close to Mars' equator.

Murray JB, Muller JP, Neukum G, Werner SC, van Gasselt S, Hauber E, Markiewicz WJ, Head JW 3rd, Foing BH, Page D, Mitchell KL, Portyankina G; HRSC Co-Investigator Team.

Nature. 2005 Mar 17;434(7031):352-6.

PMID:
15772653
5.

Growth and form of planetary seedlings: results from a microgravity aggregation experiment.

Blum J, Wurm G, Kempf S, Poppe T, Klahr H, Kozasa T, Rott M, Henning T, Dorschner J, Schräpler R, Keller HU, Markiewicz WJ, Mann I, Gustafson BA, Giovane F, Neuhaus D, Fechtig H, Grün E, Feuerbacher B, Kochan H, Ratke L, El Goresy A, Morfill G, Weidenschilling SJ, Schwehm G, Metzler K, Ip WH.

Phys Rev Lett. 2000 Sep 18;85(12):2426-9.

PMID:
10978073

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