Léiomyosarcome de la veine cave inférieure. A propos de trois observations [Leiomyosarcoma of the inferior vena cava. Three cases].

We report three new cases of leiomyosarcoma of the inferior vena cava observed between 1985 and 1990. Two of them developed in women and one in a man. The age of the patients were 56, 29 and 57 years. The three tumors have been removed completely. One patient received postoperative radio- and chemotherapy and is well 68 months after excision. One patient developed liver metastasis 18 months after resection despite chemotherapy and died after 3 years. The last one refused postoperative radio- and chemotherapy, developed massive local recurrence and pulmonary metastasis three months postoperatively, and is still alive with disease after 8 months. The diagnostic modalities of these rare tumors as well as the problems created by their surgical resection and the need for a complementary treatment are discussed.

Intra-plant variation for progress of cell division in developing oat grains : a preliminary study

Selostus: Esitutkimus kauran röyhyn sisäisestä vaihtelusta jyvän täyttymisen käynnistyessä

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.