From b4ee12e7466be0ada585185958396310e7a506e5 Mon Sep 17 00:00:00 2001 From: Sarah Foxley Date: Wed, 17 Apr 2024 15:53:55 +0100 Subject: [PATCH 1/4] Added extra fullstop --- docs/source/concepts/MatrixWorkspace.rst | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/docs/source/concepts/MatrixWorkspace.rst b/docs/source/concepts/MatrixWorkspace.rst index b593c1edc9ec..935143cd8f08 100644 --- a/docs/source/concepts/MatrixWorkspace.rst +++ b/docs/source/concepts/MatrixWorkspace.rst @@ -11,7 +11,7 @@ Matrix Workspace A Matrix Workspace is a generic name for a family which contains measured (or derived) data (Y) with associated errors (E) and an axis (X) giving information about where the measurement was made. The Matrix Workspace forms a 2D structure, more details on this will be provided below. This is the most common structure for storing data in Mantid. This covers several more detailed workspace types including: - :ref:`Workspace2D ` - A workspace for holding 2D, accumulated data in memory, this is the most commonly used to store histograms. -- :ref:`EventWorkspace ` - A workspace that retains the individual neutron event data. +- :ref:`EventWorkspace ` - A workspace that retains the individual neutron event data.. What information is in a Matrix Workspace ------------------------------------------ From 7081ddb7eddc2ddeb6f695357c5e4d08f5c54ef3 Mon Sep 17 00:00:00 2001 From: Sarah Foxley Date: Tue, 23 Apr 2024 13:00:19 +0100 Subject: [PATCH 2/4] Another full stop. --- docs/source/concepts/DiffractionCalibrationWorkspace.rst | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/docs/source/concepts/DiffractionCalibrationWorkspace.rst b/docs/source/concepts/DiffractionCalibrationWorkspace.rst index 105e6e315628..c8d69fc33478 100644 --- a/docs/source/concepts/DiffractionCalibrationWorkspace.rst +++ b/docs/source/concepts/DiffractionCalibrationWorkspace.rst @@ -26,7 +26,7 @@ The order of the rows and columns will not matter to algorithms that use the workspace. Algorithms that create the :ref:`TableWorkspace ` will use this column order with the rows sorted by ``detid`` (smallest first). Any missing column, other than ``detid``, -will be assumed to be all zeros. +will be assumed to be all zeros.. Diffraction Calibration File ============================ From 8afb91cc31089886122098f5b828cf34a37414eb Mon Sep 17 00:00:00 2001 From: Sarah Foxley Date: Wed, 24 Apr 2024 11:54:21 +0100 Subject: [PATCH 3/4] Add extra line --- docs/source/algorithms/Abins2D-v1.rst | 2 ++ 1 file changed, 2 insertions(+) diff --git a/docs/source/algorithms/Abins2D-v1.rst b/docs/source/algorithms/Abins2D-v1.rst index 795a9ab5f453..77167166a2bb 100644 --- a/docs/source/algorithms/Abins2D-v1.rst +++ b/docs/source/algorithms/Abins2D-v1.rst @@ -17,6 +17,8 @@ Description Abins2D is a plugin for Mantid which allows scientists to generate theoretical inelastic neutron scattering spectra (INS) in 2-D :math:`(|\mathbf{q}|,\omega)` space, accounting for the limitations of real-world measurements. +Add another test line here. + The intensity is calculated in the "almost-isotropic" incoherent powder-averaging approximation, as used in the 1-D :ref:`Abins ` algorithm. Different 2-D INS instruments may be selected, along with instrument parameters (incident energy, chopper settings) that determine the accessible :math:`(|\mathbf{q}|,\omega)` region and energy resolution. More information about the implemented working equations can be found :ref:`here `. From 32f40a8c1ecb69bf58e646818f66711c35cb7deb Mon Sep 17 00:00:00 2001 From: thomashampson Date: Thu, 25 Apr 2024 10:56:05 +0100 Subject: [PATCH 4/4] add test line --- docs/source/algorithms/Abins2D-v1.rst | 2 ++ 1 file changed, 2 insertions(+) diff --git a/docs/source/algorithms/Abins2D-v1.rst b/docs/source/algorithms/Abins2D-v1.rst index 77167166a2bb..a6d8a37d7d36 100644 --- a/docs/source/algorithms/Abins2D-v1.rst +++ b/docs/source/algorithms/Abins2D-v1.rst @@ -19,6 +19,8 @@ Abins2D is a plugin for Mantid which allows scientists to generate theoretical i Add another test line here. +Add another test line here too. + The intensity is calculated in the "almost-isotropic" incoherent powder-averaging approximation, as used in the 1-D :ref:`Abins ` algorithm. Different 2-D INS instruments may be selected, along with instrument parameters (incident energy, chopper settings) that determine the accessible :math:`(|\mathbf{q}|,\omega)` region and energy resolution. More information about the implemented working equations can be found :ref:`here `.