The IONO4HAS tool performance and quality is evaluated through positioning 22 different rover receivers using different techniques. Rovers are grouped
to form networks in dedicated regions (coded by colours):
Yesterday's ionospheric residuals
This test is computed from the yesterday's ionospheric modelling residuals at the rover receivers.
1 / 22
RIO1 (Logrono, Spain)
2 / 22
ZARA (Zaragoza, Spain)
3 / 22
TERU (Teruel, Spain)
4 / 22
ALBA (Albacete, Spain)
5 / 22
COBA (Córdoba, Spain)
6 / 22
VALA (Valladolid, Spain)
7 / 22
YEBE (Yebes, Spain)
8 / 22
SONS (Sonseca, Spain)
9 / 22
CACE (Cáceres, Spain)
10 / 22
WARE (Waremme, Belguim)
11 / 22
DENT (Dentergem, Belgium)
12 / 22
VLIS (Vlissingen, The Netherlands)
13 / 22
KOS1 (Kootwijk, The Netherlands)
14 / 22
MET3 (Kirkkonummi, Finland)
15 / 22
METG (Metsähovi, Finland)
16 / 22
GOP6 (Ondrejov, Czechia)
17 / 22
SJSP (São José Dos Campos, Brazil)
18 / 22
ALAR (Arapiraca, Brazil)
19 / 22
SPBO (Sao Carlos, Brazil)
20 / 22
MGLA (Lavras, Brazil)
21 / 22
PEAF (Afogados da Ingazeira, Brazil)
22 / 22
ILHA (Ilha Solteira, Brazil)
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click to see next rover ionospheric solution (all rovers).
click here to examine the distances between rovers and reference stations
Real-time rover positioning error
1 / 22
RIO1 (Logrono, Spain)
2 / 22
ZARA (Zaragoza, Spain)
3 / 22
TERU (Teruel, Spain)
4 / 22
ALBA (Albacete, Spain)
5 / 22
COBA (Córdoba, Spain)
6 / 22
VALA (Valladolid, Spain)
7 / 22
YEBE (Yebes, Spain)
8 / 22
SONS (Sonseca, Spain)
9 / 22
CACE (Cáceres, Spain)
10 / 22
WARE (Waremme, Belguim)
11 / 22
DENT (Dentergem, Belgium)
12 / 22
VLIS (Vlissingen, The Netherlands)
13 / 22
KOS1 (Kootwijk, The Netherlands)
14 / 22
MET3 (Kirkkonummi, Finland)
15 / 22
METG (Metsähovi, Finland)
16 / 22
GOP6 (Ondrejov, Czechia)
17 / 22
SJSP (São José Dos Campos, Brazil)
18 / 22
ALAR (Arapiraca, Brazil)
19 / 22
SPBO (Sao Carlos, Brazil)
20 / 22
MGLA (Lavras, Brazil)
21 / 22
PEAF (Afogados da Ingazeira, Brazil)
22 / 22
ILHA (Ilha Solteira, Brazil)
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❯
click to see next rover position error (all rovers).
click here to examine the distances between rovers and reference stations
FPPP and PPP component results
Depicted data corresponds to last 4 hours. Full reset every 2 hours
Horizontal component
Vertical component
Statistics during the last 7 days
95th Percentile
Real-time ionospheric rover solution using the unambiguous STEC residuals
These plots are generated for each rover receiver, depicting the rover solution in blue, and in red
the residues for all the other receivers within the same network, used in the IONO4HAS model.
1 / 22
RIO1 (Logrono, Spain)
2 / 22
ZARA (Zaragoza, Spain)
3 / 22
TERU (Teruel, Spain)
4 / 22
ALBA (Albacete, Spain)
5 / 22
COBA (Córdoba, Spain)
6 / 22
VALA (Valladolid, Spain)
7 / 22
YEBE (Yebes, Spain)
8 / 22
SONS (Sonseca, Spain)
9 / 22
CACE (Cáceres, Spain)
10 / 22
WARE (Waremme, Belguim)
11 / 22
DENT (Dentergem, Belgium)
12 / 22
VLIS (Vlissingen, The Netherlands)
13 / 22
KOS1 (Kootwijk, The Netherlands)
14 / 22
MET3 (Kirkkonummi, Finland)
15 / 22
METG (Metsähovi, Finland)
16 / 22
GOP6 (Ondrejov, Czechia)
17 / 22
SJSP (São José Dos Campos, Brazil)
18 / 22
ALAR (Arapiraca, Brazil)
19 / 22
SPBO (Sao Carlos, Brazil)
20 / 22
MGLA (Lavras, Brazil)
21 / 22
PEAF (Afogados da Ingazeira, Brazil)
22 / 22
ILHA (Ilha Solteira, Brazil)
❮
❯
click to see next rover position error (all rovers).
click here to examine the distances between rovers and reference stations
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