This service allows to quickly calculate geomagnetic, invariant and other coordinates for a given point at a given time.ĭeveloped in 2007. The data available can be retrieved as text tables, charts, and as archive files. This service is a mirror of NASA COHOweb project, which allows online access to data from Pioneer-10/11/Venus, Voyager-1/2, Ulysses and Helios-1/2 data. ![]() It provides access to numerous parameters of solar and Earth physics from 1969 to 2008. This service is a mirror of NASA OMNIweb project. Measurements of UV radiation of night atmosphere carried out by the “Universitetsky-Tatiana” satellite. Transient luminous events (source: Universitetsky-Tatyana) This tool is based on an earlier work by J.Shugai. SOHO is a project of international cooperation between ESA and NASA. Their work was supported by the INTAS-ESA projects 99-00727 and 03-51-6206 (coordinator: Volker Bothmer), RFBR, Astronomy state program and the Universities of Russia federal program.Ĭatalogue of solar images and data on count, surface area and average intensity of coronal holes identified in them. The APEV tool uses data retrieved from appropriate sources and compiled by Alexei Dmitriev, Andrei Zhukov and Igor Veselovsky. Spatial distributions over geographical map of trapped, quasi-trapped and precipitated electrons (300-600 keV) measured onboard of CORONAS-F and Universitetsky-Tatyana satellites in the evening-night MLT sectors.Ĭatalogue of solar events, containing coronal hole maps, DSF maps and solar wind conditions for each event. Spatial particle distribution (sources: Coronas-F and Universitetsky-Tatyana) Flux intensity is indicated by pixel color. The X axis corresponds to day-of-year, the Y axis corresponds to the L-shell value. The header contains particle type, and measurement year and month. Imagery of flux dynamics of charged particles in 2001-2005, one for every three months. Temporal charged particle distribution statistics (source: Coronas-F) X-ray flares and proton events during the last three solar cyclesīased on proton measurements onboard GOES and IMP-8, neutron monitor data and GOES X-ray measurements, this database combines information on proton events captured in near-Earth spaceĬatalogue of magnetic storms in 1998-2005 based on OMNIweb data with Dst index threshold selection capability. The database can be used for the Omniweb HTML email system.Solar flares with Hard X-rays (HXR) detected by SONG ( CORONAS-F) ĭata on solar flares detected by SONG expreiment (detection time and peak γ-ray energy channel) and soft X-ray (SXR) flare GOES characteristics. ![]() It is very simple to build attractive HTML emails and send these out to subscribers. On these for- mats, several retrieval and visualisation tools have been built, such as OMNIWeb, CDAWeb, PAPCO, SDDAS. ![]() If a visitor has subscribed to a newsletter, the CRM system is also used as a source for email marketing. They can also produce reports and export data for use in other systems. The added benefit is that the visitor is actually updating their own record.īuilt into the Omniweb CRM are several additional tools that allow our web site clients to add records themselves for clients who contact by phone. This ensures that databases are kept as clean as possible. If an existing record is found, then the details are updated and the new transaction is appended to his/her record. Rather than having multiple databases with lots of duplicated contacts, the idea is to have one contact for each customer or sales prospect with a list of all the transactions between the company and that particular contact.Įach time a visitor to one of our web sites fills in a form or checkout page their details are compared with the database. Contact Database Creating a clean database of people who interact with your web site.Ĭustomer Relationship Marketing (CRM) systems are designed to provide a single database of a company's contacts.
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