• GLE Alert Plus

    Real time Alert system for Ground Level Enhacement (GLE) events which monitors the recordings of each NM station providing data to NMDB.

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    A full physics laboratory for meteorological, renewable energy sources, CO2 effect etc.

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ESA SSA*

ESA’s Space Situational Awareness (SSA) Programme was authorised at the November 2008 Ministerial Council and formally launched on 1 January 2009. The mandate was extended at the 2012 Ministerial Council until 2019, and the programme is funded through to 2016.

The objective of the SSA programme is to support Europe's independent utilisation of, and access to, space through the provision of timely and accurate information and data regarding the space environment, and particularly regarding hazards to infrastructure in orbit and on the ground.

In general, these hazards stem from possible collisions between objects in orbit, harmful space weather and potential strikes by natural objects, such as asteroids, that cross Earth’s orbit.

SSA aims, ultimately, to enable Europe to autonomously detect, predict and assess the risk to life and property due to man-made space debris objects, reentries, in-orbit explosions and release events, in-orbit collisions, disruption of missions and satellite-based service capabilities, potential impacts of Near-Earth Objects (NEOs), and the effects of space weather phenomena on space- and ground-based infrastructure.

SSA means that Europe will know what goes on in space by acquiring the independent capability to watch for objects and natural phenomena that could harm our infrastructure.

ESA’s 1 m-diameter telescope in Tenerife discovered its fifth NEO (2013 CZ133) in February 2013. Another NEO discovered with the support of ESA’s SSA programme, the 30 m-diameter 2012 DA14, passed Earth at 27 700 km on 15 February 2013, the same day, by chance, that a 17 m-diameter NEO exploded in the sky above Chelyabinsk, Russia.

For Europe, space is a crucial region.

Space-based systems have become indispensable to many services critical to Europe’s economies and government functions, including those related to security. This dependency will only increase in the future.

NEO observations using ESA’s 1 m-diameter telescope in Tenerife will continue in 2013–16. The telescope discovered its fifth NEO (2013 CZ133) in February 2013. Another NEO discovered with the support of ESA’s SSA programme, the 30 m-diameter 2012 DA14, passed Earth at 27 700 km on 15 February 2013, the same day - by chance - that a 17 m-diameter NEO exploded in the sky above Chelyabinsk, Russia.

Any shutdown or loss of services from these systems would seriously affect an enormous range of commercial and civil activities, including commercial land, air and sea travel, maritime navigation, telecommunications, information technology and networks, broadcasting, climate monitoring and weather forecasting, to name but a few.

In the event of a disruption to space-based services or supporting infrastructure on the ground, citizens’ safety could be significantly affected and the delivery of emergency services by regional, national and European authorities could be considerably impaired.

To date, Europe’s access to information on what is happening in space has been largely dependent on non-European sources. In recent years, for example, data to trigger alerts on potential collisions between European satellites and debris objects have only come through the good will of other spacefaring nations. For this and other reasons, Europe needs an autonomous SSA capability.

Furthermore, developing existing capabilities will strengthen the competitive edge of European industry. For example, in the area of space weather, Europe already has a wealth of expertise and assets providing high-quality scientific data and, in some cases, space weather products to local customers. However, these are largely fragmented across national and institutional boundaries. A new, coordinated approach to developing space-weather applications tailored to European user needs together with the supporting research and infrastructure would strongly increase our capabilities in this area.

The programme is active in three main areas:

  1. Survey and tracking of objects in Earth orbit
    comprising active and inactive satellites, discarded launch stages and fragmentation debris that orbit Earth
  2. Monitoring space weather
    comprising particles and radiation coming from the Sun that can affect communications, navigation systems and other networks in space and on the ground
  3. Watching for NEOs
    comprising natural objects that can potentially impact Earth and cause damage, and assessing their impact risk and potential mitigation measures

To undertake these activities, the programme is federating existing assets and capabilities from ESA, European and international partners into a set of unified SSA capabilities.

These are being extended by newly developed infrastructure including databases, software tools and applications and optical survey telescopes and may include dedicated satellite missions in the future.

During the 2009–12 SSA Preparatory Phase, two new test radars were contracted from industry, one to be located in Spain and one in France, to test, validate and develop future radar search and detection techniques, a capability not currently available in Europe under civil control.

In 2013, for example, ESA’s existing Proba-2 solar observatory satellite will be shifted to the responsibility of the SSA programme, becoming in effect the first ‘SSA mission’.

New SSA coordination centres for space weather (at Space Pole, Brussels) and for NEOs (at ESA/ESRIN) are being inaugurated, and these will start providing precursor services on a test and evaluation basis. A Tasking Centre has been established at ESA/ESOC, and will begin providing a trial real-time response capability.

Much more will be done during the current Phase II period of the programme to 2016.

A crucial aspect of SSA activities is cooperation. SSA is managed directly by ESA on behalf of the Agency’s Member States, who fund the programme. SSA also includes cooperation with European national and regional authorities, including ministries of defence, national space agencies and national research establishments, particularly those with existing ground- and space-based sensors.

SSA activities are also extending Europe's long-standing cooperation with organisations in the USA, including NASA, NOAA and the US Defense Department, and with bodies such as the UN and other international agencies.

During the 2009–12 initial phase of the SSA programme, over 25 contracts were issued to industry for SSA-related work with a total value in excess of €30 million.

For example, there are eight contractors spread across four Member States working to develop and build the required test radar technology.

This represents a significant return on investment for Member States and highlights the abilities of European industry to play an active role in developing essential tracking abilities to help secure safe use of space.

SSA is enabling Europe to play a fundamental role in support of the peaceful uses of outer space by providing the international community with independent options for verifying compliance with treaties and codes of conduct.

SSA also supports international technical, regulatory and political processes by furnishing knowledge based on independent data and information. Importantly, SSA directly supports the EU Lisbon Objectives, to foster the development of new applications, new services, new jobs and new markets.

The SSA programme will help to ensure:

  • The reliability, availability and security of Europe’s space-based applications are strengthened
  • Reaffirmation of Europe’s autonomous access to space, gaining full knowledge of events in the economically and strategically important orbits near Earth
  • The peaceful uses of outer space are enhanced in cooperation with international partners
  • That European industry benefits from contracts and new, world-class competitive capabilities gained through the development of SSA infrastructure and capabilities

 

*Reference: http://www.esa.int/Our_Activities/Operations/Space_Situational_Awareness/About_SSA

A.NE.MO.S - Athens Neutron Monitor Station

We collaborated with National and Kapodistrian University of Athens Neutron Monitor Forecasting Group from 2000-2012 on project Pythagoras in order to build Athens Neutron monitor Registration System The first update happened after the ISSI workshop in 2000 in Athens, Greece a Neutron Monitor (Super 6NM-64) came back to the mighty family of the world wide Neutron Monitors with real time data from November 10, 2000.
This station is housed in a specially constructed room at the roof of the Physics building at the campus of the National and Kapodistrian University of Athens.
Athens Station unique in the Balkan area and the east part of the Mediterranean Sea. It was among the first stations (4th) in the worldwide Neutron Monitor Network provided real time data to the Internet. The station is very useful for scientific as well as educational purposes
The new modern Cosmic-Ray Station of the Athens University installed and developed with new instruments and electronics parts that made it possible to provide accurate data with resolution up to 1 sec. The whole project run under the efforts, guidance and responsibility of Assoc. Prof. Mavromichalaki and the Athens Cosmic Ray Group in co-operation with IZMIRAN group and ISNet Company.
Under the supervision of Assoc. Prof. Mavromichalaki five Phds (Gerontidou, PhD 2007; Plainaki, PhD 2007; Sarlanis, PhD 2008, Souvatzoglou, PhD 2009, Papaioannou, PhD 2010).

Since 2003 a new data processing center (Athens Neutron Monitor Data Processing Center - ANMODAP) collecting data from 23 real time NM stations together with satellite data from ACE & GOES, is operated at the Athens NM station. By this Center a real time Alert system determining the onset of the GLEs is developed by ISNet.

Some of the scientific aims of Athens Neutron Monitor

  • The energy spectrum of the cosmic-ray modulation effects (11-years and more long-term variations, 27-days, Forbush effects) where data from the sea level stations of high cutoff rigidity need to be used, can be determined. At present there is a deficit of such stations (only a few on mountains and one at the sea level - Beijing). Such stations are also necessary to obtain a rigidity spectrum of Cosmic-Ray anisotropy.
  • This station is very important for estimation the energy limit of particles in the great proton events. Frequently the upper energy of the particles accelerated at the Sun is ranged within 5-10 GeV, that is very close to the minimal energy of particles recorded in Athens.
  • This station is suitable for the study of magnetospheric effects (November, 2003).
  • This station may be used to record and study the solar neutron enhancements.
  • May be used by other stations for data corrections (e.g. snow effects-ESO Israel).


Publications and Conferences

  • H. Mavromichalaki,C. Sarlanis, G. Souvatzoglou, G. Mariatos, M. Gerontidou, C. Plainaki, A. Papaioannou, and S. Tatsis "The new Athens Center applied to Space Weather forecasting’ RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society AIP Conference Proceedings, 848, 837-846, 2006
  • H. Mavromichalaki, G. Souvatzoglou, C. Sarlanis, G. Mariatos, M. Gerontidou, A. Papaioannou, C. Plainaki, S. Tatsis, A. Belov, E. Eroshenko, V. Yanke "The new Athens Center on data processing fromthe Neutron Monitor Network in real time" First European Space Weather Week 2004, ESA/ESTEC, The Netherlands Annales Geophysicae, 23, 1-8, 2005
  • A. Papaioannou, M. Gerontidou, G. Mariatos, H. Mavromichalaki, C Plainaki "Unusually extreme cosmic ray events in July 2005’ 2nd ESA SWW (14-18 November 2005) Holland (http://esa-spaceweather.net/spweather/workshops/eswwII/)
  • H. Mavromichalaki, M. Gerontidou, G. Mariatos , C. Plainaki, A. Papaioannou, C.Sarlanis, G. Souvatzoglou, A. Belov, E. Eroshenko, V. Yanke and S. Tsitomeneas "Space Weather forecasting at the new Athens Center: The recent extreme events of January 2005" IEEE TRANSACTIONS for Nuclear Science 52, 6, 2307-2312, 2005
  • E. G. Stassinopoulos, H. Mavromichalaki,C.Sarlanis, G. Souvatzoglou and S. Tsitomeneas "A Study for an Unmanned Aerial Vehicle carrying a radiation spectrometer networked to the new Athens Center active in Space Weather Events forecasting" Proc. RADECS 2005 CONFERENCE (19-23 Sept. 2005) LN-10
  • A. V. Belov, E. A. Eroshenko, H.Mavromichalaki, A.Papaioannou, G. Mariatos, V. G. Yanke "Cosmic ray modulation in August-September 2005" Proc. 20th ECRS - 2006, Lisbon, 2006
  • Mavromichalaki, C. Plainaki, M. Gerontidou, C.Sarlanis, G. Souvatzoglou, G. Mariatos,A. Belov, E. Eroshenko, E. Klepach and V.Yanke "GLEs as a Warning Tool for Radiation Effects on Electronics and Systems: A new Alert System based on Real-Time Neutron Monitors" Proc. RADECS 2006 Workshop, Athens, 2006 IEEE TRANSACTIONS for Nuclear Science, 54, 1083 - 1088, 2007
  • H. Mavromichalaki, M. Gerontidou, C. Plainaki, A. Papaioannou, G. Mariatos, M. Papailiou, C. Sarlanis, G. Souvatzoglou "Athens Neutron Monitor Data Processing Center – ANMODAP Center" 30th ICRC 2007, Workshop, Merida, Mexico
  • H. Mavromichalaki, M. Gerontidou, C. Plainaki, A. Papaioannou, G. Mariatos, M. Papailiou, C. Sarlanis, G. Souvatzoglou "Real-time cosmic ray monitoring and analysis of GLE70 from the Athens Neutron Monitor Data Processing Center" 8th Hellenic Astronomical Conference, Thassos, September 2007 (http://www.ee.duth.gr/hac/node/659)
  • Mavromichalaki, G. Souvatzoglou, C Sarlanis, G. Mariatos, A. Belov, E. Eroshenko, V. Yanke "Real Time GLE ALERT for December 2006 at the ANMODAP center" Solar Extreme Events 2007 Symposium (Sept 2007), 87 Adv. Space Research 2007 (submitted)
  • Sarlanis C., Souvatzoglou G., Mavromichalaki H., Kartyshov V., Klepach E.,Yanke V., Yudacin K.: System of data accumulation for multidirectional muon telescopes. Proc. 29th ICRC, 2005, SH.3.6.
  • H. Mavromichalaki, M. Gerontidou, G. Mariatos, M. Papailiou, A. Papaioannou, C. Plainaki, C. Sarlanis, G. Souvatzoglou: ‘Athens Neutron Monitor Data Processing Center – ANMODAP Center’, Adv. Space Res., 44, 1237-1246, 2009
  • H. Mavromichalaki, G. Souvatzoglou, C. Sarlanis, G. Mariatos, A. Papaioannou, A. Belov, E. Eroshenko, V. Yanke: ‘Implementation of the Ground Level Enhancement Alert Software at NMDB database’, New Astronomy, 15, 744-748, 2010
  • A. Papaioannou, H. Mavromichalaki, M. Gerontidou, G. Souvatzoglou, P. Nieminen, A. Glover: 'Solar Particle Event Analysis Using the Standard Radiation Environment Monitors: Applying the Neutron Monitor's Experience', Astrophys. Space Sci. Trans., 7, 1-5, 2011
  • H. Mavromichalaki, A. Papaioannou & NMDB group: ‘Applications and usage of the real-time neutron monitor database (NMDB)’, Adv. Space Res., 47, 2210-2222, 2011
 

NHREAS

"A Very High Resolution Weather, Wave and Ship Safety Forecasting System"
G. Kallos1, E. Mavromatidis1, G.Galanis1, F. Gofa1, A. Laskaratos1, G. Korres1, G. Tompras1, G. Souvatzoglou7, C. Sarlanis7, C. Efstathiou1, K. Politis2, J. Vergados3, G. Sakelaridis4, E. Markou4, C.Tremback5 and J. Snook6

1 University of Athens, School of Physics, Division of Applied Physics
2 Hellenic Ship Registry-HSR, Piraeus, Greece
3 Innovative Technology Center –ITC S.A., Athens, Greece
4 Hellenic National Meteorological Service, Athens-HNMS, Greece
5 ATMET S.A., Boulder, CO, USA
6 CORA S. A., Boulder, CO, USA

7
ISNET, Athens, Greece

Project: New EKBAN 1.3-87
Ministry of Development – General Secretariat for Research and Technology

Project started in 1998 and ended in 2000.

More specific and we designed and implemented a mobile meteorological station that measure and trasmiting parameters through GSM/GPRS, INMARSAT B and Satelite Internet data to Hellenic National meteorological Service.
We implemented the part of server in the
Hellenic National meteorological Service too.

Coordinator: University of Athens, School of Physics, Atmospheric Modeling and Weather Forecasting Group, Assoc. Professor G. Kallos

Other Partners:
School of Physics, Oceanography Group, University of Athens
School of Physics, Telecommunications Group University of Athens
School of Informatics, University of Athens
Hellenic National Meteorological Service (HNMS)
Hellenic Ship Registry (HSR S.A.)
Strintzis Lines S.A.
Innovative Technology Center (ITC S.A.)
ISNet

SCOPE OF THE PROJECT

THE DEVELOPMENT of: A very high resolution forecasting system for weather, waves and ship safety to support the coastal transportation system between the Greek Mainland and the Aegean Islands.

The system consists of:

  • A high resolution atmospheric module (RAMS and LAPS).
  • A high resolution wave module (WAM), for Greek Seas and mainly for Saronic Gulf and Central Aegean.
  • A telecommunication module which employs advanced data transferred systems (GSM, DCS1800, INMARSAT etc. connections)
  • A data gathering and distribution module (with two parts one at HNMS and the other on board of the ships).
  • A ship stability and safety module on specific weather and sea conditions (SWAN module).

Operational use of NHREAS system:

  • Retrieval of ECMWF meteorological and SST fields for initial and boundary conditions.
  • Retrieval of all available surface observational data from surface and ship stations (NHREAS stations).
  • Retrieval of all available upper-air data.
  • The Data Assimilation System LAPS is used to prepare initial conditions based on the ECMWF gridded fields as initial guess, the surface and upper-air observations available at the HNMS and the data gathering from the telecommunication system of NHREAS.

The system produces:

  • 36-hour forecasts starting at 00:00 UTC.
  • Post-processing and preparation of graphical representations of RAMS results.
  • Usage of model results as input at the 4th generation wave model WAM for wave forecasting.
  • Post-processing and preparation of graphical representations of WAM results.
  • Update of the system’s server and web page for interactive usage.

Users (e.g. the crew of the ship):

  • Can browse at NHREAS server located at HNMS for weather and wave forecasts and at the same time they can gather the necessary data for scenario development about the safety and route to follow.
  • Telecommunication is realized through three alternative ways: GSM data service, INMARSAT class-B data transfer and satellite internet.
  • The data gathering system of HNMS downloads the data from each ship-station every 15? automatically through the telecommunications systems available at each ship.
  • The ship-stations download the data to HNMS through INMARSAT and satellite internet connections.
  • Each ship-station has extra sub modules like GPS and electronic compass for positioning and true wind calculations.
  • Conventional RAMS outputs are also available at HNMS.

The final users for the pilot implementation of the project were chosen to be the following ships:

  • BLUE STAR FERRIES «SUPER FERRY II»
  • BLUE STAR FERRIES «ITHAKI»
  • MINOAN LINES «KNOSSOS PALACE»

 

COMPUTER RESOURCES
The computational system, which is in use at HNMS for NHREAS consists of:

  • A cluster of 3 dual-CPU HP/J6000 + 1 single CPU HP/C-3000 (as Control Workstation) linked with 1GBit Switch (optical).
  • An HP/server (1GHz PENTIUM) with dial-up modems.
  • All the systems are linked with the other subsystems at HNMS through a 100 Mbit net .
  • The connection with the internet is made via the University of Athens and ECMWF.


SHIP TERMINAL STATION
The terminal station at the ships consist of two basic operational parts:

  • The sensors for the meteorological and positioning data.
  • The computer that supports: a) Two-way communications with the main server at HNMS. b) Gathering, retrieval and storage of the meteorological data and the position of the ship. c) Retrieval of weather and wave forecasted fields. d) Performance of ship stability calculations for safer and optimum navigation according to wave conditions, cruising speed and route to follow.

The meteorological mast on the "Bluestar Ithaki" deck.

We can see the anemometer, the GPS antenna, the temperature and humidity sensors, the wind sensors, the gsm antenna and the compass. The installation takes into account the sea environment in order to resist to near sea conditions and the acceleration conditions that items meet during the ship movement under different sea conditions.

THE COMPUTER SYSTEM AT THE SHIP DECK

The prototype system at “Blue Star Ithaki”. In each of three Ships installed different systems with different type of instruments and ways of communications in order to evaluate the best performance. In the later versions of the system the computer boards and the other electronics are within a box with fixed specifications and the control of the system is made through a touch-screen and track-ball system.

The parts of the ship station

The computer system

The computer system has the role of

  • Display the current meteorological conditions around the ship.
  • Storage the data that ship datalogger gather.
  • Sending gathered data every 10 minutes (1 minute measurements) to the Hellenic Meteorological Service. Later in the project datalogger has the same capability and the one system worked as backup of the other.
  • Get data and images with forecasting charts from the prediction models and display on the ship monitor

Marine type wind –gauge and wind-vane
In the picture we can see the model 05106 marine type anemometer of RM Young Company. In the project we evaluate some types of anemometers. Between them were ultrasonic and cup anemometers and wind vanes.

Compass Sensor
In the picture we can see the Flux Gate compass sensor DH0200 of Ritchie. We use some type of similar sensors from different suppliers. The use of a such sensor was critical
especially when ship was not make moves of make movements inside a harbor. In such cases the GPS sensor is useless in order to continue to have valid wind data.

GPS Sensor
You can see the marine type GPS by Koden company. We use a number of sensors in the project independent or combined with a GSM modem.

Signal Conditioning Unit
We can see the signal conditioning unit. It can handle the following sensors

  • A PT-100 thermometer
  • A voltage output Humidity sensor
  • A voltage output Barometric pressure sensor
  • A RS-232 NMEA0183 output compass sensor
  • A RS-232 NMEA0183 output gps sensor
  • A RS-232 NMEA0183 output wind sensor
  • A Voltage output wind sensor (2 inputs)
  • A pulse output cup anemometer
  • A RS-232 gsm modem

It sends its output to the Ship Computers and communicate with it in order to handle a number of situations.

RESULTS AVAILABLE AT THE NHREAS WEB SERVER (Prognosis)

Wind speed and direction
Wave direction and significant height
Wave direction and period
Temperature at 2m
Cloud coverage (percentage)
Accumulated precipitation (last 3 hours)
Wind and Wave fields for interactive retrieval from ships for the ship-safety calculations and optimal route path. These data are available for the highest resolution available of the selected location.

HESPERIA stands for:  High Energy Solar Particle Events foRecastIng and Analysis. It is an H2020 project, under PROTEC-1-2014: Space Weather

The project officially started on 01 May 2015 and will last for two years.

HESPERIA will produce two novel operational forecasting tools based upon proven concepts (UMASEP, REleASE). At the same time it will advance our understanding of the physical mechanisms that result into high-energy solar particle events (SEPs) exploiting novel datasets (FERMI/LAT/GBM; PAMELA; AMS) and it will explore the possibility to incorporate the derived results into future innovative space weather services. In order to achieve these goals HESPERIA will exploit already available large datasets stored into databases such as the Neutron Monitor Database (NMDB) and SEPServer that have been developed under FP7 projects from 2008 to 2013

The results will be openly accessible to the public through the dedicated web interface of HESPERIA and will further be posted in related servers such as NMDB and SEPServer.

The HESPERIA consortium consists of 9 partners with complementary expertise covering all aspects of the project. HESPERIA will also collaborate with a number of institutes and individuals from US and Russia, ensuring both the in depth analysis of the novel datasets to be utilized within the project and the efficient dissemination of the results to the whole space physics/space weather community.

Contact us

ISNet
Intelligent Systems Networks
Argiroupoleos 91, Argiroupolis
Athens 16451, Greece
T: +30 210 4830600
F: +30 210 4813175
Working time:
Mon-Fri: 10:00 to 18:00

Mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Partners

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Request for collaboration

Small scientific teams go for collaborations and cooperation in implementation of their activities.

ISNet is a growing scientific organization which is looking for smooth implementation of their projects.

We, the team at ISNet, are alive to the rapidly changing trends and provide customized solutions keeping in view the individual needs. We believe in developing mutually beneficial relationships. The relationship will bring mutual benefits.

Benefits of Collaboration:

We believe that together we can bring strong optimization in every project that both together could hanlde.

If you interest in send us a mail to: This email address is being protected from spambots. You need JavaScript enabled to view it.

Latest News

GLE Alert Plus

Gle Alert plus is real time system which created for SSA Space Weather Coordination Centre (SSCC).

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NMDB

The Neutron Monitor Database (NMDB) Project started in January 2008 and officially ended at January 2010. We still continue support this effort till today. The NMDB was a FP7 project.

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