UNITOV Catalogue of geoeffective CMEs

A database associating L1 Time of Arrival and Speed of an interplanetary CME to the kinematic characteristics of the corresponding CME, covering the period 1996-2020.

References

Dataset summary

internal_name:

unitov_icme_tableset

publisher:

University of Rome Tor Vergata Dept. of Physics

alph_code:

15

id_tmp:

44

short_name:

UNITOV-ICME

identifier:

aspis:/unitov/icme_tableset

dynamic:

+10kB updated every year

size:

100kB

format:

csv

type:

tableset

records_number:

213

time_start:

1997-01-01

time_stop:

2019-12-31

spatial:

IP

messenger:

Photons,Protons

spectral_min:

0

spectral_max:

0

spectral_units:

observable:

{CME, SW}

latest update:

2024-05-16 06:11:43

Columns specification

progr

column

units

type

description

1

time

UTC

datetime

datetime (1997-01-06T16:23:38) - time of the first detection of the CME in LASCO FoV

2

HPC_Tx

arcsec

float

arcsec (25.21) - Helioprojective Cartesian Longitutude: the angle relative to the plane containing the Sun-observer line and the Sun’s rotation axis, with positive values in the direction of the Sun’s west limb

3

HPC_Ty

arcsec

float

arcsec (-3.22) - Helioprojective Cartesian Latitude: the angle relative to the Sun’s equatorial plane, with positive values in the direction of the Sun’s north pole

4

HPC_distance

AU

float

AU (0.98) - the Sun-observer distance

5

CME_num

index

int

index (1) - progressive number

6

Start_Date

UTC

datetime

datetime (1997-01-06 16:23:38.000) - extimated time of the CME passage at 20 R_Sun

7

Arrival_Date

UTC

datetime

datetime (1997-01-06 16:23:38.000) - time of the CME passage at L1

8

PE_duration

hours

float

hours (22.0) - ICME Plasma Event duration at L1

9

Arrival_v

km/s

int

km/s (450) - measured velocity of the CME at L1

10

Transit_time

hours

float

hours (98.3) - time elapsed from the Start_Date and Arrival_Date

11

Transit_time_err

hours

float

hours (98.3) - error associated to the extimated transit time

12

LASCO_Date

UTC

datetime

datetime (1997-01-06 16:23:38.000) - time of the first detection of the CME in LASCO FoV

13

LASCO_v

km/s

int

km/s (459.5) - plane-of-sky velocity of the CME from LASCO images

14

LASCO_pa

deg

int

deg (263.0) - CME principal angle, counterclockwise from North

15

LASCO_da

deg

int

deg (165.0) - CME angular width

16

LASCO_halo

char

char

string (N/PH/HH/FH) - indicating halo/partial halo CME

17

v_r

km/s

float

km/s (705.35) - estimated radial velocity of the CME

18

v_r_err

km/s

float

km/s (104.89) - error associated to the radial velocity of the CME

19

Theta_source

arcsec

float

arcsec (14.92) - longitude of the most probable source of the CME on the solar disk

20

Phi_source

arcsec

float

arcsec (-25.97) - co-latitude of the most probable source of the CME on the solar disk

21

source_err

arcsec

float

arcsec (20.0) - uncertainty on the source location on the solar disk

22

POS_source_angle

deg

float

deg (64.60) - plane-of-sky angle of the source region of the CME

23

rel_wid

rad

float

rad (0.5585) - estimated deprojected CME angular width

24

Mass

g

float

g (1.8e+16) - Estimated mass of the CME

25

SW_type

char

char

char (F/S) - Solar wind type (Fast/Slow) for the ICME propagation

26

Bz

nT

int

nT (16) - z-component of the ICME magnetic field at L1

27

DST

nT

int

nT (-68.0) - minimum DST during ICME event at L1

28

v_r_stat

km/s

float

km/s (544.73) - statistical de-projection of the CME POS speed

29

Accel.

m/s^2

float

m/s^2 (8.9076) - CME acceleration between the lift-off and 20 solar radii

30

Analyitic_w

km/s

float

km/s (395.56) - solar wind value obtained via analytic inversion of the DBM equations

31

Analyitic_gamma

km^-1

float

km^-1 (3.5029e-06) -value of the drag parameter obtained via analytic inversion of the DBM equations

32

filename

char

char

string (CME_0111_param_inv.txt ) - name of the file containing PDBM information from the statistical inversion procedure

Code example

"""

This is an example script for accessing client-side ASPIS datasets.

The client is provided by the ASPISpy package and in particular the connection is resolved by the CaesarAPI class.

This example code allows the user to fetch a product from the ASPIS DB and

save it in a ready-to-use pandas.DataFrame structure.

To use this code to fetch another product, simply change

the product name and possibly the time range and columns of the dataset

(for the filtered_search method).

Notes:

- The CaesarAPI class provides a complete interface to the ASPIS DB through several methods,

each of which corresponds to a different API endpoint.

- Once CaesarAPI has been instantiated through authentication, the user can call the different methods

(e.g., CaesarAPI.download_data, CaesarAPI.filtered_search, etc. etc.).

- The import and initialization are the same for each code fragment.

"""

#### The following lines of code should be executed only once

#### during session initialization. If they are re-executed,

#### the session in ASPIS DB is recreated from scratch.

#### Once the session is initialized, the user can use of all

#### the methods provided by the CaesarAPI class.

import ASPISpy.aspis as aps

import pandas as pd

# The following lines to disable SSL certificate warning.

# Note: In this prototype version, the certificate is not available

import requests

from requests.packages.urllib3.exceptions import InsecureRequestWarning

requests.packages.urllib3.disable_warnings(InsecureRequestWarning)

# Initialize the CaesarAPI connector

api = aps.CaesarAPI(credentials={'email': '<your_email>','password': '<your_password>'})

# [INFO] user <your_email> authenticated

# Define the product to be fetched

product_name = "unitov_icme_tableset"

# FETCH THE FULL DATASET

r, df = api.get_product_detail(product_name)

# r is the full response of the request, df is the pandas.DataFrame

# which contains the dataset.

# > print(df.head())

#     id                 time     HPC_Tx     HPC_Ty  HPC_distance  CME_num  ...

# 0   0  1997-01-06T15:10:42  25.210143  -3.221796      0.983319        1   ...

# 1   1  1997-02-07T00:30:05  53.055793  -7.993757      0.986300        2   ...

# 2   2  1997-04-07T14:27:44  14.917489 -25.972924      1.001209        3   ...

# 3   3  1997-05-12T05:30:05   6.568649  21.393300      1.010308        4   ...

# 4   4  1997-05-21T21:00:53 -63.993601 -35.996400      1.012279        5   ...

# FETCH A SUBSET of <product_name>

df = api.filtered_search(prod_id=product_name,filters=['time < 2005-01-01','time > 2000-01-01'],cols=['time','bz','dst','v_r'],return_dataframe=True)

# [INFO] Executing the following query:

#     query MyQuery {

#       filtered_search(filters: [{field: "time", operator: "lt", value: "2005-01-01"}{field: "time", operator: "gt", value: "2000-01-01"}]) {

#         ... on UnitovIcmeTablesetType {

#           time

#           bz

#           dst

#           v_r

#         }

#       }

#     }

# > print(df.head())

#                   time  bz  dst      v_r

# 0  2000-01-18T17:54:05  16  -97  1132.60

# 1  2000-02-08T09:30:05   7  -25  1364.00

# 2  2000-02-10T02:30:05  13 -133  1097.20

# 3  2000-02-12T04:31:20   5  -67  1286.90

# 4  2000-02-17T19:31:23  15  -26   566.07

``