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.
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:
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:
*Reference: http://www.esa.int/Our_Activities/Operations/Space_Situational_Awareness/About_SSA
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
Publications and Conferences
"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:
Operational use of NHREAS system:
The system produces:
Users (e.g. the crew of the ship):
The final users for the pilot implementation of the project were chosen to be the following ships:
COMPUTER RESOURCES
The computational system, which is in use at HNMS for NHREAS consists of:
SHIP TERMINAL STATION
The terminal station at the ships consist of two basic operational parts:
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
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
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.
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.
Gle Alert plus is real time system which created for SSA Space Weather Coordination Centre (SSCC).
Read more...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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