Baptiste Cecconi
Corentin K. Louis
Xavier Bonnin1- 1LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon, France
- 2School of Cosmic Physics, DIAS Dunsink Observatory, Dublin Institute for Advanced Studies, Dublin, Ireland
- 3H H Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom
TFCat (Time-Frequency Catalogue) is a data interchange format based on JSON (JavaScript Object Notation), which has been initially designed for exchanging low frequency radio events and features. It defines several types of JSON objects and how they are combined to represent data related to temporal-spectral features of a time spectrogram (a.k.a., dynamic spectrum), their properties, and their temporal and spectral extents. This implementation is inheriting from the GeoJSON file format. The TFCat python library is implementing this specification and provides a software interface permitting to create, update and validate TFCat objects efficiently.
1 Introduction
At the lower end of the radio frequency domain, i.e., below ≈ 100 MHz, the electromagnetic signatures are tracers of energetic and unstable particle populations rather than atomic and molecular transitions. Such features are usually identified with their spectral-temporal (also referred to as “time-frequency”) shape in time varying spectrograms (also referred to as dynamic spectra). Such time-frequency features are related to Earth and planetary magnetospheres (magnetospheric and auroral radio emissions), Earth and planetary lightnings (electrostatic discharges), Solar activity (solar radio bursts), as well as astrophysical radio sources such as Pulsars or Fast Radio Bursts. For a review of the low frequency planetary radio emissions, see Zarka (2004). Figure 1 shows an example dynamic spectrum recorded by the Cassini/RPWS (Radio and Plasma Waves Science) instrument (Gurnett et al., 2004) displaying Solar and Terrestrial low frequency radio features.
FIGURE 1. Low frequency radio dynamic spectrum recorded by Cassini/RPWS on 1999-08-26. The spectrogram is showing Solar radio bursts as well as terrestrial auroral kilometric radiation (AKR).
Since the early 1960’s, a corpus of catalogues identifying and documenting such Jovian radio emissions (Barrow and Desch, 1980; Barrow, 1981; Leblanc et al., 1981, Leblanc et al., 1983; Aubier and Genova, 1985; Leblanc et al., 1989, Leblanc et al., 1990; Riihimaa, 1991; Leblanc et al., 1993; Marques et al., 2017), and solar radio bursts (Maxwell et al., 1963; Bernold, 1980; Kayser et al., 1988; Zhang et al., 2018) have been published, or are available online (such as the Bleien Solar Radio Data legacy web page1), providing access to: lists of event bounding boxes in the temporal-spectral plane; more refined contour shapes; or linear features. However, there was no standard exchange format, leading to difficulties in sharing and reusing such catalogues.
The TFCat (Time-Frequency Catalogue) specification has been developed with the aim of facilitating the recording, rese and processing of low frequency radio temporal-spectral events. In the past two years, several catalogues have been published using the TFCat format, and tools are now implementing interfaces on top of this specification, for labelling observations, displaying catalogues, or even using the catalogue shapes to select and process observational data (Cecconi et al., 2021a; Fogg et al., 2021; Louis et al., 2021; Taubenschuss et al., 2021; Wu et al., 2021, Wu et al., 2022b, Wu et al., 2022a).
In this paper, we will present the needs and use cases identified in the preliminary stages of the TFCat specification project. We then detail the proposed catalogue model and its implementation. The associated python library is also presented, with a series of examples and applications.
2 Needs and use cases
The MASER service (Measuring, Analysing and Simulating Emissions in the Radio range) is a science ready toolkit for low frequency radio astronomy (Cecconi et al., 2020). During its inception, the storing, processing and sharing of labelled features in radio frequency dynamic spectra has been identified as one of the major community needs. The main complexity is the shape representation of the features, as a series of coordinates in the temporal-spectral plane. The MASER team has thus explored various applicable solutions based on existing tools and standards in the astronomy, heliophysics and Earth sciences.
The astronomy community has developed an interoperability framework called the “Virtual Observatory” and maintained by the IVOA (International Virtual Observatory Alliance, https://ivoa.net). They define many standards allowing to build complex interoperable data infrastructures. For the purpose of catalogues and events, three standards are applicable: the VOTable (Virtual Observatory Table) format (Ochsenbein et al., 2019), the VOEvent (Virtual Observatory Event) model (Seaman et al., 2011) and the STC (Space-Time Coordinate) model (Rots, 2007) or its upcoming successor2. Those formats and models are very well designed for astronomical catalogues and events, including time intervals, spectral ranges, spatial regions on the sky (most often using Right Ascension (RA) and Declination (Dec) coordinates). However, there is currently no way to build and share more detailed geometries mixing temporal and spectral coordinates using those tools. The heliophysics community has also defined a set of standards including a heliophysics event list (HPEventList3), which is using CSV (comma separated values) and VOTable as serialization formats. The same restriction applies as for the astronomy applications.
The description of two-dimensional (2D) geometries or coverage information can be done using various tools and methods. The solar physics community has been using the “chaincodes” method (see, e.g., the SunPy implementation4), which describes a 2D geometry specifying a starting point on an image and then listing the pixel per pixel path along the feature contour. Such implementation is computationally very efficient, but is providing geometry in pixel coordinates, requiring the access to the original data (and metadata) to reuse the described feature. In the astronomy framework, the MOC (HEALPix –Hierarchical Equal Area isoLatitude Pixelisation– Multi-Order Coverage map) standard (Fernique et al., 2019) is currently allowing to describe spatial and temporal complex coverage maps, however the spectral dimension is not considered yet in the standard. Finally in the Earth science community, feature geometries are using the GeoJSON format (Butler et al., 2016). This format is using geographic coordinates to describe features and proposes several classes of features (such as points, segments or polygons).
In order to facilitate the adoption by catalogue providers (e.g., authors of publications), the selected solution must be easy to implement and should avoid dependencies on too specific software. On the user side, the same statement applies with the other requirements that it should be easy for tool and science platform developers to implement the solution.
Besides the description of the temporal-spectral feature geometries, it shall be possible to set additional properties for each feature (e.g., a label, an identifier linking to the original observation, or any property or statistical quantity related to the observed feature). Such properties shall be defined properly, so that users can reuse and process them. Furthermore, the catalogue shall contain metadata covering the scope of the catalogue itself (such as authors, references, a title). Metadata on the source datasets, from which the feature catalogue is derived, should also be referenced. Finally the temporal and spectral axes must be properly defined within the catalogue.
3 Proposed catalogue model
The TFCat model provides a way to describe a series of features referenced by their coordinates (or set of coordinates) in the temporal-spectral plane, as observed from a radio instrument (a ground based telescope or onboard a spacecraft), and identified by an agent (a scientist or a software). Each feature of the catalogue is defined by a set of temporal and spectral coordinates, and a geometry type. Features can have additional properties, depending on the science case, which content shall be defined in the catalogue. The temporal and spectral coordinate frame in use in the catalogue shall be defined uniquely in a catalogue file, or identified by unique coordinate system name. The catalogue can have general properties (e.g., header type metadata). The TFCat base model elements are:
• TFCat Geometry—There are 7 types of TFCat Geometry: Point, MultiPoint, LineString, MultiLineString, Polygon, MultiPolygon, with an additional GeometryCollection, which is a set of any of the six other geometry types. Each geometry is composed of a set of coordinate pairs. A LineString is defined by a list of connected Point features, forming a continuous path. A Polygon is defined by a closed list of connected Point features, forming a closed contour. The feature type definitions are inspired from the GeoJSON specification (Butler et al., 2016).
• TFCat Feature—A TFCat Feature contains one or several TFCat Geometries, and a set of properties, provided as a set of (key, value) pairs.
• TFCat Field—A TFCat Field is defining the TFCat feature properties. Its minimal content includes a name, a description, a data type and a UCD (Unified Content Descriptors) (Cecconi et al., 2021b). It may also include a unit [following the VOUnit –Virtual Observatory Unit–specification (Derriere et al., 2014)], or a set of allowed values, when applicable.
• TFCat Property—A TFCat Property is a (key, value) pair. There are two types of TFCat Properties:
• TFCat Feature Property—TFCat feature properties are used in a TFCat Feature. They must be defined with a corresponding TFCat Field.
• TFCat Collection Property—TFCat collection properties are used in a TFCat Feature Collection. They should provide generic information on the catalogue, such as: title, authors, reference, instrument, etc.
• TFCat Coordinate Reference System—A TFCat Coordination Reference System (CRS) contains a description of the time axis, a description of the spectral axis, and a reference position. The TFCat CRS could be of three types: name, link or local.
3.1 Javascript object notation implementation
The TFCat model has been implemented using the JSON format (Bray, 2014), reusing the structure of the GeoJSON specification. The TFCat JSON specification is available (Cecconi et al., 2022b). The specification is maintained on a git repository5. When applicable the astronomy standards have been implemented (UCD (Preite Martinez et al., 2018), VOUnit (Derriere et al., 2014), and list of known keywords, like, e.g., reference positions).
The TFCat CRS specification aligns on GeoJSON CRS definition. Currently, the TFCat CRS must be defined in the TFCat object instance. However, a set of predefined time axis are available within the specification (e.g., unix, jd, mjd, etc).
3.2 Catalogue validation
A JSON Schema document6 has been prepared to validate the catalogues. However, the JSON schema only covers part of the specification, since some constraints could not be implemented therein (like, e.g., the need to have a TFCat Field defined for each TFCat Feature Property). An example of TFCat validation using the JSON schema is provided in Section 4.1.
A full validator (based on the TFCat specification) has been implemented in STILTS7 (Starlink Tables Infrastructure Library Tool Set, Taylor, 2006), version 3.4-7 or later.
This java-based tool can be called on the command line:
Listing 1. Validating a TFCat file
1 java -classpath stilts.jar uk.ac.starlink.tfcat.
Validate <filename.json>
4 Time-frequency catalogue python library
Since the TFCat JSON implementation is closely inheriting from GeoJSON, many tools from the Earth science community can be reused. First, the TFCat python library8 has been developed starting from the code of a python GeoJSON library9. The TFCat library also makes use of the shapely library10, which can be used for managing and processing TFCat features in general.
4.1 Creating a time-frequency catalogue feature collection
The two main elements required to start preparing a TFCat feature collection is the choice of the CRS and the list of feature geometries (with its set of time and spectral coordinates). In the following code snippet, a CRS object is created with a time axis using the unix timestamp representation, a spectral axis (frequency in kHz) and a reference position set to the Juno spacecraft.
Listing 2. Example CRS definition
1 from tfcat import CRS
2 crs = CRS({
3 "type": "local",
4 "properties": {
5 "name": "Time-Frequency",
6 "time_coords_id": "unix",
7 "spectral_coords": {
8 "type": "frequency",
9 "unit": "kHz",
10 },
11 "ref_position_id": "juno",
12 }
13 })
In the following example, we create a TFCat feature with a TFCat Polygon geometry and two custom feature properties called feature_type and integrated_flux_density. The names and values of feature properties are not constrained by the TFCat specification. However, the specification requires to include TFCat Fields defining any TFCat feature property that may be included in a Feature. The set of coordinates are available in two variables called tt and ff, containing respectively the time coordinates (as a unix timestamp), and the frequency coordinates (in kHz). Note, that a Polygon geometry requires that the last coordinate point of the input sequence should be the same as the first one (closed polygon condition). It also requires that the segments forming the polygon are not crossing over (no cross-over condition). The polygon must also be curled counter-clockwise. We use the shapely package to check the latter condition.
Listing 3. Creating a TFCat Polygon
1 from tfcat import Polygon, Feature
2 from shapely.geometry import LinearRing
3 # packing coordinates into a list
4 coords = list(zip(tt, ff))
5 # checking if list of coordinates is curled in the direct trigonometric sense (counter-clockwise)
6 if not LinearRing(coords).is_ccw:
7 coords = coords[::-1]
8 # creating the TFCat Feature
9 feature = Feature(
10 geometry=Polygon([coords]),
11 properties={
12 "feature_type": "Io-A",
13 "integrated_flux_density": 1.22e-19,
14 },
15 )
Each properties must be defined at the main level of the feature collection object, using a set of TFCat Field objects, as shown below.
Listing 4. Defining Fields
1 fields = {
2 "feature_type": {
3 "info": "Feature Type",
4 "datatype": "str",
5 "ucd": "meta.id",
6 },
7 "integrated_flux_density": {
8 "info": "Integrated Flux Density",
9 "datatype": "float",
10 "ucd": "phot.flux.density;stat.mean",
11 "unit": "W m-2 Hz-1",
12 }
13 }
The feature collection can also include collection-level properties, listing global metadata for the collection, such as the author, the instrument, etc. The next code snippet shows a set of collection level properties. We recommend to use keywords compliant with the EPNcore (Europlanet core) metadata dictionary (Erard et al., 2022) for Solar System related collections. A data_source_reference property may be included to refer to the data collection used to derive the catalogue. The value of the data source reference should be a DOI if it is available for the progenitor resource. However, any type of well-known community reference could be used, such as, e.g., a SPASE (Roberts et al., 2018) resource identifier or a NASA/PDS (Planetary Data System) identifier11. For authors, we recommend to use a list of dictionaries containing GivenName, FamilyName, ORCID and Affiliation (using ROR12 when possible). The current version of the TFCat specification does not define mandatory properties, nor does it define the object type of collection level properties. This may be implemented in a future version, in order to improve the interoperability and reusability.
Listing 5. Defining collection level properties
1 properties = {
2 "instrument_host_name": "Juno"
3 "instrument_name": "Waves",
4 "title": "Catalogue of Juno Radio emissions",
5 "authors": [
6 {
7 "GivenName": "Corentin K.",
8 "FamilyName": "Louis",
9 "ORCID": "https://orcid.org/0000-0002-9552-8822",
10 "Affiliation": "https://ror.org/051sx6d27"
11 },
12 ],
13 "target_name": "Jupiter",
14 "target_class": "planet",
15 "target_region": "magnetosphere",
16 "feature_name": "radio emissions",
17 "bib_reference": "10.1029/2021JA029435",
18 "data_source_ref": "http://doi.org/10.25935/6jg4-mk86",
19 "publisher": "PADC/MASER",
20 "version": "1.0",
21 }
Finally, the collection can be built, assuming a list of features is available in an object called features. The JSON schema URI can also be referenced. The default value is set to the latest released TFCat JSON schema URI (i.e., https://voparis-ns.obspm.fr/maser/tfcat/v1.0/schema# at the time of writing).
Listing 6. Finalizing a TFCat collection
1 from tfcat import FeatureCollection
2 SCHEMA_URI = "https://voparis-ns.obspm.fr/maser/tfcat/v1.0/schema#"
3 # creating the collection
4 collection = FeatureCollection(
5 schema=SCHEMA_URI,
6 features=features,
7 properties=properties,
8 fields=fields,
9 crs=crs,
10 )
The TFCat collection can then be checked against the JSON Schema.
Listing 7. Validating a TFCat collection
1 from tfcat.validate import validate
2 validate(collection)
Writing the collection into a file is straightforward, since the TFCat module implements the same interfaces as the json python module for file system interactions (i.e., dump(), dumps(), load(), loads() methods):
Listing 8. Dumping into File
1 # write out the collection on disk
2 from tfcat import dump
3 filename = "tfcat.json"
4 with open(filename, "w") as f:
5 dump(collection, f)
4.2 Loading a time-frequency catalogue feature collection
The TFCat module also provides capabilities to load TFCat JSON files from the local file system, or from a remote location:
Listing 9. Loading local or remote TFCat file
1 from tfcat import TFCat
2 local_cat = TFCat.from_file(<filepath>)
3 remote_cat = TFCat.from_url(<URL>)
In the following example, we load TFCat file available in Taubenschuss et al. (2021). The script first displays the coordinate reference system (using the crs property), and the geometry type of the first feature. It then plots the two first features of the catalogue (see Figure 2), and then shows the use of the temporal and spectral converters, which can be used to load the time-frequency coordinates as an astropy.time.Time object for the time component, and an astropy.units.Quantity for the spectral component.
FIGURE 2. Example plots from Listing 10.
Listing 10. Example script
1 from tfcat import TFCat
2 tf_file = ’cassini_faraday_patches_2006.json’
3 cat = TFCat.from_file(tf_file)
4 cat.crs
5 # {"properties": {"name": "Time-Frequency", "ref_position_id": "cassini-orbiter",
6 # "spectral_coords": {"type": "frequency", "unit": "Hz"}, "time_coords_id": "unix"},
7 # "type": "local"}
8 cat.feature(0).geometry.type
9 # ’MultiPoint’
10 cat.plot_feature(0)
11 cat.plot_feature(1)
12 cat.crs.time_converter(cat.feature(0).tmin).isot
13 # ’2006-09-12T09:02:26.750’
14 cat.crs.spectral_converter(cat.feature(0).fmax)
15 ;# <Quantity 43469. Hz>
4.3 Module installation and dependencies
The TFCat module is distributed under MIT licence. The module dependencies are limited to a small set of external modules: astropy (Astropy Collaboration et al., 2022), matplotlib (Hunter, 2007), shapely (Gillies et al., 2007) and jsonschema (Berman et al., 2022). It is available on PyPI13 and can thus be installed with pip:
Listing 11. Install TFCat with pip
1 pip install tfcat
5 Applications
TFCat has already been used in several published data collections (Cecconi et al., 2021b; Fogg et al., 2021; Louis et al., 2021; Taubenschuss et al., 2021; Smith et al., 2022; Wu et al., 2021, Wu et al., 2022b, Wu et al., 2022a). In order to showcase the capabilities of the TFCat format and its python implementation, 3 Jupyter notebook tutorials have been prepared, and are available in Cecconi et al. (2022a) 14:
• TFCat MultiPoint feature and feature processing (MultiPoint_Example.ipynb) is showing how to use TFCat together with shapely to process a MultiPoint geometry into a Polygon.
• TFCat MultiPolygon feature and data filtering example (MultiPolygon_Example.ipynb) is showing how to use TFCat together with shapely and das2 (Piker et al., 2019) to use a MultiPolygon geometry to select data and perform statistical analysis.
• TFCat Multiple Catalogue Example (Multiple_Catalogue_Example.ipynb) is showing how to compare two catalogues containing features derived from the same physical events.
The TFCat model and python library are used in the SPectrogram Analysis and Cataloguing Environment (SPACE) Labelling Tool (Louis et al., 2022). TFCat features can also be loaded and displayed in Autoplot (Faden et al., 2010). Full support is not currently available, but an example Jython script is provided15 by the Autoplot team.
6 Conclusion and future prospects
The TFCat format and its associated Python library are providing the low frequency radio astronomy community with a novel tool enabling interoperability and reusability of temporal-spectral features. The published catalogues are demonstrating its usefulness through various use cases. The proposed notebooks are showing its usability. Furthermore, the accessibility is guaranteed by the open access policies of the current TFCat catalogue publishers. The findability of the TFCat catalogues can be implemented using existing community data discovery interfaces (such as EPN-TAP (Erard et al., 2022) for Solar System sciences). In order to enable the findability of the features, an implementation using the TAP Table Access Protocol, (Dowler et al., 2019), is under study.
The TFCat format is now used in publications and tools to store, share and process temporal-spectra features. The GeoJSON inherited specification allows to reuse python based libraries (such as shapely) for processing the geometries. At Observatoire de Paris, the MASER team is integrating TFCat in their machine learning pipelines related to planetary and solar radio emissions, as well as in their radio data flagging pipelines (for excluding radio frequency interferences in the data processing).
The TFCat collection properties are currently loosely defined: (a) the list of keywords is not defined in the TFCat specification; and (b) there is no metadata associated to them. This will be improved in a future major version, since this would require to refactor the already published collection. The specification foreseen for the TFCat collection properties would have the same definition as the TFCat Field items, with an additional value attribute, containing the value of the property. Such specification would improve TFCat reusability and interoperability, and it would make the format more compatible with other formats, such as VOTable.
Discussions are also ongoing with other communities dealing with temporal-spectral features, such as transient astrophysics (e.g., pulsars or fast radio bursts studies), meteor radio echoes, or even space based in-situ particle observations, for which the spectral axis would then represent an energy, mass or mass per charge axis.
Data availability statement
The original contributions presented in the study are included in the article, further inquiries can be directed to the corresponding author.
Author contributions
BC and CL developed the TFCat specification. BC developed the TFCat JSON Schema. BC, XB, and AL developed the TFCat python library. MT reviewed the TFCat specification, and developed the TFCat validator. BC wrote the first version of the papier. XB, AL, and MT commented and proofread the manuscript.
Funding
The Europlanet 2024 Research Infrastructure (EPN2024RI) project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149. CKL’s work at DIAS is supported by the Science Foundation Ireland Grant 18/FRL/6199. BC and MT’s contributions for this study are supported by the EPN2024RI project. BC, XB, and AL acknowledge additional funding provided in France by the Centre National d’Études Spatiales (CNES), and Action Spécifique Observatoire Virtuel (ASOV). Support from Paris Astronomical Data Centre (PADC) is acknowledged.
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.
Footnotes
1http://soleil.i4ds.ch/solarradio/.
2Astronomical Coordinates and Coordinate Systems (2021) Proposed IVOA Recommendation. Version 1.0. https://www.ivoa.net/documents/Coords/20210924/index.html.
3Heliophysics Event List: https://spase-group.org/docs/conventions/HDMC-Event-List-Specification-v1.0.4.pdf.
4SunPy.Chaincode: https://docs.sunpy.org/en/stable/generated/api/sunpy.net.helio.Chaincode.html.
5TFCat specification: https://gitlab.obspm.fr/maser/catalogues/catalogue-format.
6TFCat JSON Schema v1.0: https://voparis-ns.obspm.fr/maser/tfcat/v1.0/schema#.
7STILTS website: http://www.starlink.ac.uk/stilts/.
8TFCat Python library: https://gitlab.obspm.fr/maser/catalogues/tfcat.
9GeoJSON: https://github.com/jazzband/geojson.
10shapely: https://shapely.readthedocs.io/en/stable/.
11Citing PDS4 Data: https://pds.nasa.gov/datastandards/citing/.
12Research Organisation Registry: https://ror.org.
13https://pypi.org/project/TFCat/.
14https://doi.org/10.25935/qwpa-7t05.
15Autoplot Jython script: https://github.com/autoplot/scripts/tree/master/formats/tfcat.
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Keywords: radioastronomy, data format, python library, catalog, JSON
Citation: Cecconi B, Louis CK, Bonnin X, Loh A and Taylor MB (2023) Time-frequency catalogue: JSON implementation and python library. Front. Astron. Space Sci. 9:1049677. doi: 10.3389/fspas.2022.1049677
Received: 20 September 2022; Accepted: 07 November 2022;
Published: 09 February 2023.
Edited by:
K.-Michael Aye, Freie Universität Berlin, GermanyReviewed by:
Pablo Gutiérrez-Marqués, Max Planck Institute for Solar System Research, GermanyHamood Ur Rehman, University of Okara, Pakistan
Copyright © 2023 Cecconi, Louis, Bonnin, Loh and Taylor. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Baptiste Cecconi, YmFwdGlzdGUuY2VjY29uaUBvYnNlcnZhdG9pcmVkZXBhcmlzLnBzbC5ldQ==